The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with light diffusing outwards. There is little evidence of spiral arm structure or distinct features. The galaxy appears to be largely spheroidal, with a high degree of circularity. The color suggests a population of older stars, with a bias toward the redder end of the spectrum. The galaxy's overall structure suggests it is a relatively undisturbed system, with no obvious signs of major mergers or tidal interactions, however there is potentially some sign of a minor disturbance. Based on its estimated size, it's a smaller galaxy, though still substantial. The apparent lack of blue light suggests a low rate of recent star formation within the galaxy.
