NGC 871

NGC 871 is a barred spiral galaxy in the Aries constellation. Its discovery and first description was realized by William Herschel on October 14, 1784 and the findings made public through his Catalogue of Nebulae and Clusters of Stars in 1786.
By using the galaxies' radial velocities and distances as a grouping factor, astronomers assign this galaxy to LGG 53 along with 8 other members.

Galaxy group NGC 871/6/7

At the current epoch, most galaxies can be found in medium-density group environments, where tidal interactions play an important role in galactic evolution. Several nearby, gas-rich groups exhibit clear signs of these interactions, giving the opportunity for scientists to study how galaxies are formed and interact with each other.
In 2012 astronomers conducted an extensive survey to measure the Hl emissions from NGC 871 and other galaxies in LGG 53, using the Giant Metrewave Radio Telescope and Canada–France–Hawaii Telescope. This galaxy group first attracted attention due to its gas-rich interaction as well as harboring AGC 749170, a galaxy with a mass of ~ M_☉. This group resides in a common HI distribution with a total HI mass of M_hl 6 x 10 M_☉. Such a massive structure is very rare in the local Universe and each large spiral in NGC 871/6/7 seems to exceeds this value.
The study suggests seven of the eight gas-rich detections contain stellar components and appear to be standard dark-matter dominated galaxies that were built during the epoch of galaxy assembly. AGC 749170 however is probably the result of major mergers and very active tidal interaction, resulting in the massive structure we can observe today.