The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light profile suggests a gradual decrease in luminosity from the core outwards, indicative of an older stellar population. There is a slight elongation, but overall, the shape is primarily round, indicating a system without significant recent mergers or tidal disruptions. Faint, diffuse light surrounds the main body of the galaxy, possibly representing a halo of older stars. There are no prominent dust lanes or spiral arm structures visible in this observation.
