The galaxy presents as a centrally concentrated, elliptical-like system. The light profile exhibits a smooth, diffuse character with a notable absence of distinct spiral arms or a prominent disk structure. There is a subtle color gradient detectable, with the central region appearing somewhat yellower compared to the slightly bluer outer regions, potentially indicating varying stellar populations with an older population towards the center. The overall shape appears largely undisturbed, suggesting a relative lack of recent major mergers or significant tidal interactions. There is a possibility of minor disturbances in the outer regions, though this requires further investigation. The galaxy appears relatively quiescent in terms of star formation activity.
