The galaxy presents a centrally concentrated luminosity profile, with a somewhat elliptical morphology. The core region exhibits a yellowish-white hue, suggestive of an older stellar population dominating that area. Moving outward from the core, a bluer, more diffuse halo is observed. This halo appears relatively smooth. The galaxy is likely undergoing some star formation, although likely at a moderate rate. There is evidence of a minor tidal disturbance, which could be indicative of a minor merger event in the recent past. The overall structure suggests a transitionary phase in its evolution.
