The galaxy presents as a disturbed system, exhibiting clear signs of tidal interactions and potentially an ongoing merger. A luminous central core, appearing somewhat smooth, is surrounded by a more diffuse halo. This halo displays asymmetry, with one side appearing extended and less defined than the other, suggesting the presence of tidal tails or streams resulting from gravitational interactions. Overall the galaxy is bright, exhibiting a bluish hue. There are no clearly defined spiral arms or a distinct disk structure. The galaxy appears to be relatively compact, with the majority of its light concentrated in the central region and the disturbed halo extending outwards.
