This galaxy presents as an elliptical-type galaxy, exhibiting a smooth, centrally concentrated light profile. The core region is bright and ellipsoidal. The light gradually decreases in intensity moving outwards from the center, with no apparent spiral arm structures or prominent dust lanes. Overall, the galaxy appears moderately elliptical in shape, showing a deviation from a perfect circular form. It exhibits a yellowish-red hue, suggesting a population dominated by older stars and a relative lack of recent star formation activity. No signs of tidal disturbances or ongoing mergers are visibly detected, leading to the assessment that it appears relatively undisturbed.
