The galaxy presents a largely elliptical morphology, appearing quite smooth and lacking any readily discernible spiral arm structure. The light distribution is concentrated towards the center, with a gradual decrease in intensity moving outwards. The core region exhibits a yellowish hue, suggesting a population of older stars. The outer regions appear fainter and exhibit a slightly bluer tint, possibly indicating the presence of some younger stars, but not indicative of significant ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of tidal interactions or recent mergers. Overall, the galaxy seems to be a relatively massive, evolved system with a low star formation rate.
