This galaxy presents an elliptical or lenticular morphology, with a generally smooth light profile. The galaxy exhibits a concentrated central bulge, appearing yellow or orange. The color indicates a population dominated by older stars. There is a notable lack of discernible spiral arm structure. Faint tidal features or minor disturbances are potentially present, though the image resolution limits conclusive identification. There is a possibility this system is in the process of a minor merger event or has experienced a merger in the past. The galaxy appears relatively compact, possessing a moderate angular size.