The galaxy presents a complex morphology, indicative of potential interactions or recent merger events. The central region appears diffuse and disturbed, with faint, elongated tidal features extending outwards. The overall color is slightly blue, which may suggest ongoing or recent star formation activity, particularly in the disturbed regions. There is no evidence of a smooth or dominant bulge component. Instead, the light distribution is irregular. The galaxy's morphology is suggestive of a system undergoing dynamical evolution.
