The galaxy presents as a somewhat diffuse, elongated structure, with a roughly elliptical morphology. The light distribution appears relatively smooth overall, however it is not entirely homogeneous. Hints of asymmetry are present in the light distribution. There is evidence of internal structure or possible tidal distortions; the system is either undergoing a relatively late-stage merger or possibly experiencing the effects of a recent interaction. The bluer hue on one side suggests the presence of a population of younger, hotter stars which can be found where star formation is occurring.
