The galaxy appears to be a relatively smooth, elliptical galaxy, with a noticeable central bulge that gradually fades into a more diffuse halo. There is a slight elongation in its shape, suggesting it is not perfectly spherical. A subtle hint of bluer light is present in the outer regions, possibly indicating some level of recent or ongoing star formation, although the dominant color is indicative of an older stellar population. There may be some minor disturbances evident in its shape, and possibly signs of past interaction or a minor merger event. No strong spiral arm structures or dust lanes are apparent in the image. The overall luminosity suggests it is a fairly massive galaxy.
