The galaxy presents as a relatively smooth, elliptical-shaped object. It appears to be an early-type galaxy exhibiting a notable central bulge that gradually fades into a diffuse halo. The bulge displays a yellowish-white hue, likely indicating a population of older, cooler stars. There is little evidence of spiral arm structure or significant dust lanes. The outer regions of the galaxy appear less defined, with a gradual decrease in luminosity towards the edges. No distinct features indicative of recent or ongoing major mergers are readily apparent, although there might be minor disturbances in the outer halo region. The galaxy's color suggests a lower rate of current star formation and a predominantly older stellar population.
