The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that graduates outwards into a less intense halo. Coloration suggests a predominantly older stellar population throughout the galaxy, based on the orange-ish hue. There is a subtle indication of a disc structure that may have once been present. No strong evidence of spiral arms or significant dust lanes are visible within the image. The overall appearance is consistent with an early-type galaxy. There is some slight disturbance visible on the outer edges, possibly indicating a minor merger that may have happened in the past. The overall shape of the galaxy is close to round.
