The galaxy presents as a centrally concentrated object. The light is generally smooth and elliptical, with a slight elongation. The core is the brightest region and appears almost spheroidal, with the light gradually diminishing outwards. There may be hints of spiral structure at the outer edges, but no defined arms are visible. The overall color suggests a relatively old stellar population, with little ongoing star formation. There is no evidence of any major mergers or tidal disturbances. There is perhaps some minor asymmetry. The object appears to be a relatively quiescent galaxy.
