The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with a gradual decrease in luminosity extending outwards. The color is primarily yellowish-white, suggesting a population of older stars and a relatively low rate of on-going star formation. There is little to no evidence of spiral arm structure or prominent dust lanes. The galaxy is approximately 5 kpc in radius.

The overall morphology indicates that this galaxy is an early-type system that has likely undergone significant evolution and quiescent star formation history. It is a very massive galaxy.
