The galaxy exhibits a moderately bright central bulge that appears relatively smooth, with a diffuse glow surrounding it. There is evidence of a possible disk structure, though it is not sharply defined. Some indications of merging or tidal disruption are present, suggesting the galaxy may be interacting with another galaxy or has undergone a merger in the past. The central region is slightly elongated in shape, and there appears to be a redder region in the center. The color gradient suggests possible ongoing star formation.
