The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology with a slight elongation. The core displays a bright, diffuse glow, suggesting a high concentration of stars or an active galactic nucleus. There is a subtle color gradient across the galaxy, with the central region appearing yellower and the outer regions showing slightly bluer tints. This color difference may indicate variations in stellar populations or dust content, with older stars or higher dust concentrations residing in the core. Faint extended light is observed surrounding the main body of the galaxy, hinting at a possible halo of stars or tidal debris from past interactions. There appears to be a minor disturbance to the morphology on one side of the galaxy, possibly from the early stages of a minor merger. The overall impression is that of a massive galaxy that has largely completed its star formation, but shows signs of some recent activity.
