This galaxy presents as a fairly elliptical, possibly disk-dominated, system. The core is very bright and centrally concentrated. There is a smooth, diffuse halo extending outwards from the central bulge, diminishing in intensity with increasing radius. Faint disturbances, like a faint tidal tail, may be present but difficult to determine based on image quality alone. The overall color is redder, indicative of an older stellar population, although there may be some bluer regions suggesting some recent star formation. Based on the smooth morphology, it may represent a transition object. Overall, the galaxy has an intermediate size and shows no indication of major mergers in the recent past.