The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with a gradual decrease in luminosity outwards. Color gradients suggest a predominantly older stellar population, appearing redder in the central regions and slightly bluer toward the outer edges. There's a hint of asymmetry, but overall the object appears largely undisturbed, with no obvious tidal features or major distortions indicative of recent mergers. The light distribution is quite compact, consistent with an early-type galaxy morphology.
