Messier 85

Messier 85 is a lenticular galaxy, or elliptical galaxy for other authors, in the Coma Berenices constellation. It is 60 million light-years away, and has a diameter of about across.
Pierre Méchain discovered M85 in 1781. It is within the outskirts of the Virgo Cluster, and is relatively isolated.

Properties

M85 is extremely poor in neutral hydrogen and has a very complex outer structure with shells and ripples that are thought to have been caused by a merger with another galaxy that took place between 4 and 7 billion years ago, as well as a relatively young stellar population on its centermost region, some of it in a ring, that may have been created by a late starburst. Like other massive, early-type galaxies, it has different populations of globular clusters. Aside from the typical "red" and "blue" populations, there is also a population with intermediate colors and an even redder population. It is likely transitioning from being a lenticular galaxy into an elliptical galaxy.
While indirect methods imply that Messier 85 should contain a central supermassive black hole of around 100 million solar masses,
velocity dispersion observations imply that the galaxy may entirely lack a central massive black hole.
M85 is interacting with the nearby spiral galaxy NGC 4394, and a small elliptical galaxy called MCG 3-32-38.
Compared to other early-type galaxies, M85 emits a relatively smaller proportion of X-rays.

Two supernovae and one luminous red nova have been observed in M85:

SN 1960R, was discovered by Howard S. Gates on 20 December 1960, and independently discovered by Leonida Rosino on 18 January 1961.
M85 OT2006-1 was discovered on the outskirts of the galaxy, by the Lick Observatory Supernova Search on 7 January 2006. It was classified as a luminous red nova, the first to be identified as such.
SN 2020nlb was discovered by the ATLAS telescope in Hawaii on 25 June 2020. This supernova got as bright as magnitude 12.