The galaxy appears as a centrally concentrated object, exhibiting a diffuse, extended halo of light. Its color profile is generally blue-white in the center and becomes redder in the outer regions. The galaxy appears to possess a generally smooth morphology, but with some asymmetry. There is evidence of tidal distortions on the galaxy, as well as evidence of ongoing or recent mergers. Although largely smooth, the galaxy shows subtle features suggestive of a possible disk component.
