The galaxy appears as a faint, diffuse object. Its morphology is suggestive of a relatively smooth structure, potentially elliptical or lenticular, with only a slight hint of a disk-like component. There is a possibility of minor tidal disturbances or faint features that would point to a past interaction or minor merger event. The object's color profile suggests a predominantly older stellar population, as indicated by the relatively red appearance. The galaxy is small. There is no evidence of a strong central bulge or active galactic nucleus. The light is not uniform.
