The galaxy exhibits a complex morphology indicative of an ongoing or recent merger event. The central region is dominated by a bright, diffuse bulge, but it appears elongated with multiple fainter components surrounding it. A distinct disk structure is difficult to discern, but hints of tidal features such as tails or bridges are apparent, suggesting gravitational interaction. Star formation activity appears to be present, based on the overall color and brightness of some regions, although the bulk of the galaxy presents as relatively quiescent. The system is likely a significant mass galaxy undergoing major morphological transformation.
