The galaxy presents a somewhat amorphous structure with a moderate radial extent. The light distribution is not entirely uniform, indicating potential substructures within the system. A hint of a spiral arm structure is present, with an offset central bulge, suggesting a possible interaction or past merger event. A faint arm extends from the right of the galaxy, with a potential disturbance, though not clear. The overall appearance suggests a galaxy in the process of merging. There does not seem to be much dust. 