The galaxy presents as a relatively smooth, elliptical-like structure. There is a bright, concentrated central bulge, which is yellow, that comprises the bulk of the galaxy's light output. The galaxy is quite round in appearance. There is a very faint, diffuse halo surrounding the central bulge, which has a slightly bluer hue, suggesting the presence of some younger stellar populations, however, overall the galaxy seems to be relatively quiescent. There is no apparent evidence of spiral arm structure or active star formation regions. The galaxy appears isolated, with no obvious signs of tidal interactions or ongoing mergers. 
