This galaxy appears to be a merging system or a galaxy with significant tidal disturbances. The main body of the galaxy exhibits a smooth, centrally concentrated light distribution indicative of an elliptical morphology or a dominant bulge component. Its light is relatively red, implying an older stellar population with minimal ongoing star formation. There is an amorphous halo of fainter light extending outward from the central region.

Distinct from the primary body, there are some blue concentrations. These might signify areas of active star formation triggered by the interactions. The overall structure is quite irregular. Some of the bluer components might not be part of the galaxy itself, but it is likely there has been at least one merger.
