The galaxy presents a generally elliptical morphology, appearing moderately smooth in structure. The central bulge exhibits a bright, concentrated luminosity. A faint, diffuse halo or disk-like structure is suspected surrounding the central region, though this is difficult to resolve with certainty. Faint features are seen which could indicate possible minor disturbances. The galaxy presents a red-shifted color profile. There is evidence that the galaxy may be interacting or undergoing a merger with smaller objects in the field.
