The galaxy presents as a fairly smooth, elliptical morphology, though it does not appear perfectly spherical. There is a slight elongation, but it is tending towards round. The central region exhibits a significantly higher surface brightness, with a yellow-white hue, indicating an older stellar population. The light appears consistent with that of a massive galaxy. The outer regions exhibit a lower surface brightness with some redder zones. There is little evidence of spiral arms or prominent dust lanes, though there is a very slight disk-like structure to it. There are no distinct tidal features or signs of major ongoing mergers, although a minor disturbance cannot be ruled out.
