List of galaxies
There are an estimated 100 billion galaxies in all of the observable universe.
On the order of 100,000 galaxies make up the Local Supercluster, and about 51 galaxies are in the Local Group.
The first attempts at systematic catalogues of galaxies were made in the 1960s, with the Catalogue of Galaxies and Clusters of Galaxies listing 29,418 galaxies and galaxy clusters, and with the Morphological Catalogue of Galaxies, a putatively complete list of galaxies with photographic magnitude above 15, listing 30,642. In the 1980s, the Lyons Groups of Galaxies listed 485 galaxy groups with 3,933 member galaxies. Galaxy Zoo is a project aiming at a more comprehensive list: launched in July 2007, it has classified over one million galaxy images from The Sloan Digital Sky Survey, The Hubble Space Telescope and the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey.
Named galaxies
This is a list of galaxies that are well known by something other than an entry in a catalog or list, or a set of coordinates, or a systematic designation.| Image | Galaxy | Constellation | Origin of name | Notes |
| Alcyoneus | Lynx | A low-exitation, Fanaroff and Riley Class II radio galaxy, one of the largest discovered. | ||
| Andromeda I | Andromeda | Andromeda I was named because the galaxy is in the constellation Andromeda | Andromeda I is a dwarf spheroidal galaxy about 2.40 million light-years away in the constellation Andromeda. Andromeda I is part of the local group of galaxies and a satellite galaxy of the Andromeda Galaxy. It is roughly 3.5 degrees south and slightly east of M31. As of 2005, it is the closest known dSph companion to M31 at an estimated projected distance of ~40 kpc or ~150,000 light-years. | |
| Andromeda Galaxy | Andromeda | Andromeda, which is shortened from "Andromeda Galaxy", gets its name from the area of the sky in which it appears, the constellation of Andromeda. | Andromeda is the closest big galaxy to the Milky Way and is expected to collide with the Milky Way around 4.5 billion years from now. The two will eventually merge into a single new galaxy called Milkdromeda According to simulations, this object would probably be a giant elliptical galaxy, but with a centre showing less stellar density than current elliptical galaxies. | |
| Ambartsumian's Knot | Ursa Major | Appearance is similar to Ambartsumian's knot | NGC 3561, also known as Arp 105, is a pair of interacting galaxies NGC 3561A and NGC 3561B within the galaxy cluster Abell 1185 in Ursa Major. It was discovered by British astronomer John Herschel on 30 March 1827. Its common name is "the Guitar" and contains a small tidal dwarf galaxy known as Ambartsumian's Knot that is believed to be the remnant of the extensive tidal tail pulled out of one of the galaxies. | |
| Antennae Galaxies | Corvus | Appearance is similar to an insect's antennae. | Two colliding galaxies | |
| Backward Galaxy | Centaurus | It appears to rotate backwards, as the tips of the spiral arms point in the direction of rotation. | ||
| Barnard's Galaxy | Named after Edward Emerson Barnard. | |||
| Bear Paw Galaxy | Lynx | It resembles the appearance of a bear's claw. | Also known as "Bear Claw Galaxy." | |
| Black Eye Galaxy | Coma Berenices | It has a spectacular dark band of absorbing dust in front of the galaxy's bright nucleus, giving rise to its nicknames of the "Black Eye" or "Evil Eye" galaxy. | Also known as "Sleeping Beauty Galaxy." | |
| Blinking Galaxy | Serpens | Its difficulty of viewing in a small telescope and tendency to go in and out of view. | - | |
| Bode's Galaxy | Ursa Major | Named for Johann Elert Bode who discovered this galaxy in 1774. | Also known as Messier 81. The largest galaxy in the M81 Group. It harbors a supermassive black hole 70 million times the mass of the Sun. | |
| Butterfly Galaxies | Virgo | Looks are similar to a butterfly. | ||
| Cartwheel Galaxy | Sculptor | Its visual appearance is similar to that of a spoked cartwheel. | The largest in the Cartwheel Galaxy group, made up of four spiral galaxies | |
| Cigar Galaxy | Ursa Major | Appears similar in shape to a cigar. | Also known as Messier 82 or M82 | |
| Circinus Galaxy | Circinus | Named after the constellation it is located in. | ||
| Cocoon Galaxy | Canes Venatici | Its resemblance in shape to a cocoon | ||
| Coma Pinwheel Galaxy | Coma Berenices | Named after its resemblance to the Pinwheel Galaxy and its location in the Coma Berenices constellation. | Also known as Messier 99 or M99 | |
| Comet Galaxy | Sculptor | This galaxy is named after its unusual appearance, looking like a comet. | The comet effect is caused by tidal stripping by its galaxy cluster, Abell 2667. | |
| Condor Galaxy | Pavo | Named after a condor, a type of vulture that is one of the largest flying birds. | The largest known spiral galaxy, it has a diameter of over. It is tidally disturbed by the smaller lenticular galaxy IC 4970. | |
| Sextans | The name of this galaxy is based on a Redshift measurement of nearly 7. | Galaxy Cosmos [Redshift 7] is reported to be the brightest of distant galaxies and to contain some of the earliest first stars that produced the chemical elements needed for the later formation of planets and life as we know it. | ||
| Dusty Hand Galaxy | Camelopardalis | Named after the dust lanes and spiral arms of the galaxy. | ||
| Eye of God | Eridanus | Named after its structural appearance | A prototype for multi-arm spiral galaxies | |
| Eye of Sauron | Canes Venatici | Due to its resemblance to the Eye of Sauron from The [Lord of the Rings |The Lord of the Rings]. | ||
| Fireworks Galaxy | Cygnus and Cepheus | Due to its bright and spotty appearance | Active starburst galaxy | |
| Fried Egg Galaxy | Pegasus | Due to its similar appearance to a fried egg | - | |
| Godzilla Galaxy | Perseus | Its extremely large size | - | |
| Helix Galaxy | Ursa Major | Its shape resembles a helix | - | |
| Grasshopper | Lynx | Named after its appearance to a grasshopper | Two colliding galaxies | |
| Hidden Galaxy | Camelopardalis | The difficulty in observing this object makes it 'hidden' though it can readily be detected even with binoculars. | ||
| Hockey Stick Galaxies | Canes Venatici | Its elongated and curved appearance resembles a hockey stick. | Also known as Crowbar Galaxy | |
| Hoag's Object | Serpens Caput | This is named after Art Hoag, who discovered this ring galaxy. | It is of the subtype Hoag-type galaxy, and may in fact be a polar-ring galaxy with the ring in the plane of rotation of the central object. | |
| Knife Edge Galaxy | Draco | Named after its thin shape, similar to knife's edge. | - | |
| Large Magellanic Cloud | Dorado/Mensa | Named after Ferdinand Magellan | This is the fourth-largest galaxy in the Local Group, and forms a pair with the SMC, and from recent research, may not be part of the Milky Way system of satellites at all. | |
| Lindsay-Shapley Ring | Volans | Named after its discoverer, Eric Lindsay, his professor Harlow Shapley, and its nature as a ring galaxy. | The ring is the result of collision with another galaxy | |
| Little Sombrero Galaxy | Pegasus | Named after its similarity to the Sombrero Galaxy. | ||
| Malin 1 | Coma Berenices | Discovered and named by David Malin. | ||
| Meathook Galaxy | Volans | After its appearance resembling a meathook. | - | |
| Medusa Merger | Ursa Major | Ejected dust from the merging galaxies is said to look like the snakes that the Gorgon Medusa from Greek mythology had on her head. | ||
| Sculptor Dwarf Galaxy | Sculptor | Similar to the Sculpture Galaxies | Also known as Sculptor Dwarf Elliptical Galaxy, Sculptor Dwarf Spheroidal Galaxy, and formerly as the Sculptor System | |
| Mice Galaxies | Coma Berenices | Appearance is similar to a mouse. | ||
| Small Magellanic Cloud | Tucana | Named after Ferdinand Magellan | This forms a pair with the LMC, and from recent research, may not be part of the Milky Way system of satellites at all. | |
| Mayall's Object | Ursa Major | This is named after Nicholas Mayall, of the Lick Observatory, who discovered it. | Also called VV 32 and Arp 148, this is a very peculiar looking object, and is likely to be not one galaxy, but two galaxies undergoing a collision. Event in images is a spindle shape and a ring shape. | |
| Milky Way | Sagittarius | The appearance from Earth of the galaxy—a band of light | The galaxy containing the Sun and its Solar System, and therefore Earth. | |
| Needle Galaxy | Coma Berenices | Named due to its slender appearance. | Also known as Caldwell 38 | |
| Wolf-Lundmark-Melotte | Cetus | Named for the three astronomers instrumental in its discovery and identification. | ||
| Paramecium Galaxy | Pegasus | Named after its appearance to the organism Paramecium | It is included in the Atlas of Peculiar Galaxies in the category galaxies with detached segments. | |
| Peekaboo Galaxy | Hydra | Galaxy was hidden behind a relatively fast-moving foreground star and became observable when the star moved aside. | Galaxy, relatively nearby, is considered one of the most metal-poor, least chemically enriched, and seemingly primordial, galaxies known. | |
| Pinwheel Galaxy | Ursa Major | Similar in appearance to a pinwheel . | Also known as Messier 101 or M101 | |
| Porphyrion | Draco | |||
| Porpoise Galaxy | Hydra | Its appearance resembles a porpoise | Also known as the Penguin Galaxy | |
| Sculptor Galaxy | Sculptor | Named after its location in the Sculptor Constellation. Also called the Silver Dollar or Silver Coin Galaxy, because of its light and circular appearance. | Also known as the Silver Coin, Silver Dollar Galaxy or Caldwell 65 | |
| Skyrocket Galaxy | Ursa Major | Its resemblance to a July 4th skyrocket | - | |
| Sombrero Galaxy | Virgo | Similar in appearance to a sombrero. | Also known as Messier Object 104 or M104 | |
| Southern Pinwheel Galaxy | Hydra | Named after its resemblance to the Pinwheel Galaxy and its location in the southern celestial hemisphere. | ||
| Spider Galaxy | Boötes | Named after its appearance of a spider | ||
| Spiderweb Galaxy | Hydra | Its irregular shape and continuous structure resembles a spiderweb. | ||
| Starfish Galaxy | Ophiuchus | Similar in appearance to a starfish. | Merger of 3 galaxies | |
| Sunflower Galaxy | Canes Venatici | Similar in appearance to a sunflower. | ||
| Tadpole Galaxy | Draco | The name comes from the resemblance of the galaxy to a tadpole. | This shape resulted from tidal interaction that drew out a long tidal tail. | |
| Topsy Turvy Galaxy | Reticulum | The disorganized and chaotic appearance makes it look topsy turvy. | - | |
| Triangulum Galaxy | Triangulum | Named after its location within the Triangulum constellation. | ||
| UFO Galaxy | Lynx | Named after its resemblance to a UFO. | - | |
| Whale Galaxy | Canes Venatici | Named after its supposed resemblance to a whale. | - | |
| Whirlpool Galaxy | Canes Venatici | From the whirlpool appearance this gravitationally disturbed galaxy exhibits. |
Naked-eye galaxies
This is a list of galaxies that are visible to the naked eye, for at the very least, keen-eyed observers in a very dark-sky environment that is high in altitude, during clear and stable weather.| Galaxy | Apparent Magnitude | Distance | Constellation | Notes |
| Milky Way | −6.5 | 0 | Sagittarius | This is the galaxy containing the Sun and its Solar System, and therefore Earth. Most things visible to the naked eye in the sky are part of it, including the Milky Way composing the Zone of Avoidance. |
| Large Magellanic Cloud | 0.9 | Dorado/Mensa | Visible only from the southern hemisphere. It is also the brightest patch of nebulosity in the sky. | |
| Small Magellanic Cloud | 2.7 | Tucana | Visible only from the southern hemisphere. | |
| Andromeda Galaxy | 3.4 | Andromeda | Once called the Great Andromeda Nebula, it is situated in the Andromeda constellation. | |
| Triangulum Galaxy | 5.7 | Triangulum | Being a diffuse object, its visibility is strongly affected by even small amounts of light pollution, ranging from easily visible in direct vision in truly dark skies to a difficult averted vision object in rural/suburban skies. | |
| Centaurus A | 6.84 | Centaurus | Centaurus A has been spotted with the naked eye by Stephen James O'Meara. | |
| Bode's Galaxy | 6.94 | Ursa Major | Highly experienced amateur astronomers may be able to see Messier 81 under exceptional observing conditions. |
- Sagittarius Dwarf Spheroidal Galaxy is not listed, because it is not discernible as being a separate galaxy in the sky.
Observational firsts
| First | Galaxy | Constellation | Year | Notes |
| First spiral galaxy | Whirlpool Galaxy | Canes Venatici | 1845 | Lord William Parsons, Earl of Rosse discovered the first spiral nebula from observing M51. |
| Notion of galaxy | Milky Way & Andromeda Galaxy | Sagittarius & Andromeda | 1923 | Recognition of the Milky Way and the Andromeda nebula as two separate galaxies by Edwin Hubble. |
| First Seyfert galaxy | NGC 1068 | Cetus | 1943 | The characteristics of Seyfert galaxies were first observed in M77 in 1908; however, Seyferts were defined as a class in 1943. |
| First radio galaxy | Cygnus A | Cygnus | 1951 | Of several items, then called radio stars, Cygnus A was identified with a distant galaxy, being the first of many radio stars to become a radio galaxy. |
| First quasar | 3C 273 | Virgo | 1962 | 3C273 was the first quasar with its redshift determined, and by some considered the first quasar. |
| First quasar | 3C 48 | Triangulum | 1960 | 3C48 was the first "radio-star" with an unreadable spectrum, and by others considered the first quasar. |
| First superluminal galactic jet | 3C 279 | Virgo | 1971 | The jet is emitted by a quasar |
| First low surface brightness galaxy | Malin 1 | Coma Berenices | 1986 | Malin 1 was the first verified LSB galaxy. LSB galaxies had been first theorized in 1976. |
| First superluminal jet from a Seyfert | III Zw 2 | Pisces | 2000 |
Prototypes
This is a list of galaxies that became prototypes for a class of galaxies.| Class | Galaxy | Constellation | Date | Notes |
| BL Lac object | BL Lacertae | Lacerta | This AGN was originally catalogued as a variable star, and "stars" of its type are considered BL Lac objects. | |
| Hoag-type Galaxy | Hoag's Object | Serpens Caput | This is the prototype Hoag-type ring galaxy | |
| Giant LSB galaxy | Malin 1 | Coma Berenices | 1986 | |
| FR II radio galaxy | Cygnus A | Cygnus | 1951 | |
| Starburst galaxy | Cigar Galaxy | Ursa Major | ||
| Flocculent spiral galaxy | NGC 2841 | Ursa Major |
Closest and most distant-known galaxies by type
| Title | Galaxy | Constellation | Distance | Notes |
| Closest galaxy | Ursa Major III | Ursa Major | 32,600 light-years | A proposed dwarf galaxy known as the Canis Major Overdensity may lie closer at 25,000 light-years, however its status as a galaxy is disputed. |
| Most distant galaxy | MoM-z14 | Sextans | z=14.44 | Existed 280 million years after the Big Bang. |
| Closest quasar | Markarian 231 | Ursa Major | z=0.0415 | Sometimes classified as a Type-2 Seyfert galaxy, though mostly considered to be the nearest quasar. |
| Most distant quasar | UHZ1 | Sculptor | z=10.1 | Gravitationally lensed quasar behind Pandora's Cluster. It is also the first quasar observed beyond a redshift of 10. |
| Closest radio galaxy | Centaurus A | Centaurus | 13.7 Mly | |
| Most distant radio galaxy | ILT J2336+1842 | Pegasus | z=6.6 | Another radio galaxy, GLEAM J0917-0012, may either lie at z=2.01 or as distant as z=8.21. |
| Closest Seyfert galaxy | Circinus Galaxy | Circinus | 13 Mly | Closest undisputed Seyfert galaxy. It has been proposed that the nearby dwarf galaxy NGC 185 may also be a Seyfert, though this status has been disputed. |
| Most distant Seyfert galaxy | HSC 0921+0007 | Hydra | z=6.56 | Seyfert 1 galaxy; also a low-luminosity quasar. |
| Closest blazar | Markarian 421 | Ursa Major | z=0.030 | This is a BL Lac object. |
| Most distant-known blazar | Q0906+6930 | Ursa Major | z=5.47 | This is a flat spectrum radio-loud quasar-type blazar. |
| Closest BL Lac object | Centaurus A | Centaurus | 13.7 Mly | Misaligned BL Lac nucleus. Also the closest radio galaxy |
| Most distant BL Lac object | FIRST J233153.20+112952.11 | Pegasus | z=6.57 | |
| Closest LINER | ||||
| Most distant LINER | z= | |||
| Closest LIRG | ||||
| Most distant LIRG | z= | |||
| Closest ULIRG | IC 1127 | Serpens Caput | z=0.018 | |
| Most distant ULIRG | z= | |||
| Closest starburst galaxy | IC 10 | Cassiopeia | A mild starburst galaxy, this is the only such galaxy within the Local Group. | |
| Most distant starburst galaxy | SPT 0243-49 | Horologium | z=5.698 | |
| Most distant spiral galaxy | Zhúlóng | Sextans | z=5.2 |
Closest galaxies
| Title | Galaxy | Date | Distance | Notes |
| Nearest galaxy | Milky Way | always | 0 | This is the galaxy containing the Sun and its Solar System, and therefore Earth. |
| Nearest galaxy to the Milky Way | Sagittarius Dwarf Spheroidal Galaxy | 1994 | 0.070 Mly | The closest, undisputed galaxy. The disputed dwarf galaxy Canis Major Overdensity is even closer at 25,000 light-years. |
| Nearest dwarf galaxy | Sagittarius Dwarf Spheroidal Galaxy | 1994 | 0.070 Mly | |
| Nearest major galaxy to the Milky Way | Andromeda Galaxy | always | 2.54 Mly | First identified as a separate galaxy in 1923 |
| Nearest giant galaxy | Maffei 1 | 1967 | 11 Mly | Nearest major elliptical galaxy to the Milky Way |
Most distant galaxies
| Title | Galaxy | Date | Redshift | Notes |
| Most remote galaxy of any type, confirmed | MoM-z14 | 2025 | z=14.44 | As of its announcement in May 2025. |
| Most remote quasar | UHZ1 | 2023 | z=10.3 | As of its announcement in 2023. |
| Most distant Lyman-break galaxy | MoM-z14 | 2025 | z=14.44 |
Timeline notes
- MACS0647-JD, discovered in 2012, with z=10.7, does not appear on this list because it has not been confirmed with a spectroscopic redshift.
- UDFy-38135539, discovered in 2009, with z=8.6, does not appear on this list because its claimed redshift is disputed. Follow-up observations have failed to replicate the cited redshift measurement.
- A1689-zD1, discovered in 2008, with z=7.6, does not appear on this list because it has not been confirmed with a spectroscopic redshift.
- Abell 68 c1 and Abell 2219 c1, discovered in 2007, with z=9, do not appear on this list because they have not been confirmed.
- IOK4 and IOK5, discovered in 2007, with z=7, do not appear on this list because they have not been confirmed with a spectroscopic redshift.
- Abell 1835 IR1916, discovered in 2004, with z=10.0, does not appear on this list because its claimed redshift is disputed. Some follow-up observations have failed to find the object at all.
- STIS 123627+621755, discovered in 1999, with z=6.68, does not appear on this list because its redshift was based on an erroneous interpretation of an oxygen emission line as a hydrogen emission line.
- BR1202-0725 LAE, discovered in 1998 at z=5.64 does not appear on the list because it was not definitively pinned. BR1202-0725 refers to a quasar that the Lyman alpha emitting galaxy is near. The quasar itself lies at z=4.6947
- BR2237-0607 LA1 and BR2237-0607 LA2 were found at z=4.55 while investigating around the quasar BR2237-0607 in 1996. Neither of these appear on the list because they were not definitively pinned down at the time. The quasar itself lies at z=4.558
- Two absorption dropouts in the spectrum of quasar BR 1202-07 were found, one in early 1996, another later in 1996. Neither of these appear on the list because they were not definitively pinned down at the time. The early one was at z=4.38, the later one at z=4.687, the quasar itself lies at z=4.695
- In 1986, a gravitationally lensed galaxy forming a blue arc was found lensed by galaxy cluster CL 2224-02. However, its redshift was only determined in 1991, at z=2.237, by which time, it would no longer be the most distant galaxy known.
- An absorption drop was discovered in 1985 in the light spectrum of quasar PKS 1614+051 at z=3.21 This does not appear on the list because it was not definitively fixed down. At the time, it was claimed to be the first non-QSO galaxy found beyond redshift 3. The quasar itself is at z=3.197
- In 1975, 3C 123 was incorrectly determined to lie at z=0.637.
- From 1964 to 1997, the title of most distant object in the universe was held by a succession of quasars. That list is available at list of quasars.
- In 1958, clusters Cl 0024+1654 and Cl 1447+2619 were estimated to have redshifts of z=0.29 and z=0.35, respectively. However, no galaxy was spectroscopically determined.
Galaxies by brightness and power
| Title | Galaxy | Data | Notes |
| Intrinsically brightest galaxy | Baby Boom Galaxy | Starburst galaxy located 12 billion light-years away | |
| Brightest galaxy to the naked eye | Large Magellanic Cloud | Apparent magnitude 0.6 | This galaxy has high surface brightness combined with high apparent brightness. |
| Intrinsically faintest galaxy | Ursa Major III | Absolute magnitude +2.2 | This does not include dark galaxies. |
| Lowest surface brightness galaxy | Andromeda IX | ||
| Most luminous galaxy | WISE J224607.57−052635.0 | As of 21 May 2015, WISE-J224607.57-052635.0-20150521 is the most luminous galaxy discovered and releases 10,000 times more energy than the Milky Way galaxy, although smaller. Nearly 100 percent of the light escaping from this dusty galaxy is Infrared radiation. | |
| Brightest distant galaxy | Cosmos Redshift 7 | Galaxy Cosmos Redshift 7 is reported to be the brightest of distant galaxies and to contain some of the earliest first stars that produced the chemical elements needed for the later formation of planets and life as we know it. |
Galaxies by mass and density
| Title | Galaxy | Data | Notes |
| Least massive galaxy | This is not considered a star cluster, as it is held together by the gravitational effects of dark matter rather than just the mutual attraction of the constituent stars, gas and black holes. | ||
| Most massive galaxy | Central galaxy in Abell 3827, 1.4 Gly distant. | ||
| Most dense galaxy | This is an ultra-compact dwarf galaxy | ||
| Least dense galaxy | |||
| Most massive spiral galaxy | The preceding most massive spiral was UGC 12591 | ||
| Least massive galaxy with globular |
Galaxies by size
| Title | Galaxy | Constellation | Diameter | Estimation method | Notes |
| Smallest known galaxy | Ursa Major III | Ursa Major | Half-light radius | A Milky Way satellite dwarf galaxy. | |
| Largest known galaxy | ESO 383-76 | Centaurus | 90% total B-light | Central galaxy of Abell 3571 | |
| Largest spiral galaxy | NGC 6872 | Pavo | D25.5 isophote | Interacting galaxy, stripped by IC 4970. | |
| Largest irregular galaxy | UGC 6697 | Leo | D25 isophote | Disrupted spiral-like galaxy, possible jellyfish galaxy. | |
| Largest lenticular galaxy | ESO 248-6 | Eridanus | 90% total B-light | Central galaxy of Abell 3112. | |
| Largest starburst galaxy | Abell 2125 BCG | Ursa Minor | 2MASS K-band total mag | ||
| Largest radio galaxy | TXS 0033+252 | Andromeda |
Interacting galaxies
| Galaxies | Data | Notes |
| The Magellanic Clouds are being tidally disrupted by the Milky Way Galaxy, resulting in the Magellanic Stream drawing a tidal tail away from the LMC and SMC, and the Magellanic Bridge drawing material from the clouds to the Milky Way galaxy. | ||
| The smaller galaxy NGC 5195 is tidally interacting with the larger Whirlpool Galaxy, creating its grand design spiral galaxy architecture. | ||
| These three galaxies interact with each other and draw out tidal tails, which are dense enough to form star clusters. The bridge of gas between these galaxies is known as Arp's Loop. | ||
| NGC 6872 is a barred spiral galaxy with a grand design spiral nucleus, and distinct well-formed outer barred-spiral architecture, caused by tidal interaction with satellite galaxy IC 4970. | ||
| Tadpole Galaxy | The Tadpole Galaxy tidally interacted with another galaxy in a close encounter, and remains slightly disrupted, with a long tidal tail. |
| Galaxies | Data | Notes |
| Arp 299 | These two galaxies have recently collided and are now both barred irregular galaxies. |
| Galaxies | Data | Notes |
| Mayall's Object | This is a pair of galaxies, one which punched through the other, resulting in a ring galaxy. |
Galaxy mergers
| Galaxies | Data | Notes |
| Antennae Galaxies | 2 galaxies | Two spiral galaxies currently starting a collision, tidally interacting, and in the process of merger. |
| Eyes Galaxies | 2 galaxies | Two galaxies which have interacted or still interacting via an off-center collision, both had interacted with M86 in the past. |
| Butterfly Galaxies | 2 galaxies | Two spiral galaxies in the process of starting to merge. |
| Mice Galaxies | 2 galaxies | Two spiral galaxies currently tidally interacting and in the process of merger. |
| NGC 520 | 2 galaxies | Two spiral galaxies undergoing collision, in the process of merger. |
| NGC 2207 and IC 2163 | 2 galaxies | These are two spiral galaxies starting to collide, in the process of merger. |
| NGC 5090 and NGC 5091 | 2 galaxies | These two galaxies are in the process of colliding and merging. |
| NGC 7318 | 2 galaxies | These are two starting to collide |
| Four galaxies in CL0958+4702 | 4 galaxies | These four near-equals at the core of galaxy cluster CL 0958+4702 are in the process of merging. |
| Galaxy protocluster LBG-2377 | z=3.03 | This was announced as the most distant galaxy merger ever discovered. It is expected that this proto-cluster of galaxies will merge to form a brightest cluster galaxy, and become the core of a larger galaxy cluster. |
| Galaxy protocluster SPT2349-56 | z=4.3 | This protocluster is located at 12.4 billion light years from the Earth. Each of these galaxies are forming stars at 1000 times that of the Milky Way, nicknamed the Dusty Red Core. |
| Galaxy | Data | Notes |
| Starfish Galaxy | This recently coalesced galaxy still has two prominent nuclei. |
| Disintegrating Galaxy | Consuming Galaxy | Notes |
| Canis Major Dwarf Galaxy | Milky Way Galaxy | The Monoceros Ring is thought to be the tidal tail of the disrupted CMa dg. |
| Virgo Stellar Stream | Milky Way Galaxy | This is thought to be a completely disrupted dwarf galaxy. |
| Sagittarius Dwarf Elliptical Galaxy | Milky Way Galaxy | M54 is thought to be the core of this dwarf galaxy. |
| Defunct Galaxy | Destroyer | Notes |
| Omega Centauri | Milky Way Galaxy | This is now categorized a globular cluster of the Milky Way. However, it is considered the core of a dwarf galaxy that the Milky Way cannibalized. |
| Mayall II | Andromeda Galaxy | This is now categorized a globular cluster of Andromeda. However, it is considered the core of a dwarf galaxy that Andromeda cannibalized. |
| Gaia Sausage | Milky Way Galaxy | It is now considered a remnant of a dwarf galaxy that collided with the Milky Way about 8-11 billion years ago. It is the last major merger of the Milky Way in its lifetime. |
Galaxies with some other notable feature
| Galaxy name | Distance | Constellation | Property | Notes |
| SDSS J081421.68+522410 | Lynx | Giant radio lobes | Also termed Alcyoneus. Its radio lobes are some of the largest known structure made by a single galaxy. | |
| M87 | Virgo | This is the central galaxy of the Virgo Cluster, the central cluster of the Local Supercluster It contains the first black hole ever imaged, in April 2019, by the Event Horizon Telescope. | ||
| M102 | Draco | This galaxy cannot be definitively identified, with the most likely candidate being NGC 5866, and a good chance of it being a misidentification of M101. Other candidates have also been suggested. | ||
| NGC 2770 | Lynx | "Supernova Factory" | NGC 2770 is referred to as the "Supernova Factory" due to three recent supernovae occurring within it. | |
| Arp 122 | Arp 122 is a collision of NGC 6040 and PGC 56942 or NGC 6039. | |||
| NGC 3314 | Hydra | exact visual alignment | This is a pair of spiral galaxies, one superimposed on another, at two separate and distinct ranges, and unrelated to each other. It is a rare chance visual alignment. | |
| ESO 137-001 | Triangulum Australe | "tail" feature | Lying in the galaxy cluster Abell 3627, this galaxy is being stripped of its gas by the pressure of the intracluster medium, due to its high speed traversal through the cluster, and is leaving a high density tail with large amounts of star formation. The tail features the largest amount of star formation outside of a galaxy seen so far. The galaxy has the appearance of a comet, with the head being the galaxy, and a tail of gas and stars. | |
| Comet Galaxy | Sculptor | interacting with a galaxy cluster | Lying in galaxy cluster Abell 2667, this spiral galaxy is being tidally stripped of stars and gas through its high speed traversal through the cluster, having the appearance of a comet. | |
| 4C +37.11 | 230 Mpc | Perseus | Least separation between binary central black holes, at | OJ 287 has an inferred pair with a 12-year orbital period, and thus would be much closer than 4C 37.11's pair. |
| SDSS J150636.30+540220.9 | z = 0.608 | Boötes | Most efficient star production | Most extreme example in the list of moderate-redshift galaxies with the highest density starbursts yet observed found in the Wide-field [Infrared Survey Explorer] data. |
| Cosmos Redshift 7 | z = 6.604 | Sextans | Brightest distant galaxy | Galaxy Cosmos Redshift 7 is reported to be the brightest of distant galaxies and to contain some of the earliest first stars that produced the chemical elements needed for the later formation of planets and life as we know it. |
| RUBIES-UDS-QG-z7 | z = 7.29 | Cetus | Earliest known massive quiescent galaxy | This galaxy is reported to be the most distant and therefore earliest massive galaxy where star formation stopped, contrary to expectations based on current models of galaxy formation. |
| AMORE6 | z = 5.725 | Sculptor | Most pristine galaxy | This galaxy is reported to be very metal poor, with the oxygen abundance of 12+log < 5.8, or <0.12% of Solar abundance, measured via JWST spectroscopy. This metallicity measurement is the lowest in the literature, making it the most pristine galaxy to date. |