The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing mostly round. There is a bright core region, which suggests a concentration of stars or possible presence of an active galactic nucleus, though no distinct features are discernable at this resolution to confirm this. The galaxy’s color is slightly more yellow/reddish than blue, which indicates a population of older stars. Faint extended light is detected around the central region, smoothly fading into the background sky. No distinct spiral arms or bar structures are visible. There appears to be minimal evidence of any ongoing major merger activity or significant tidal disturbances, although it shows some minor asymmetries, indicating past interactions or ongoing processes. Overall, the galaxy appears as a relatively evolved system.
