The galaxy presents as a relatively smooth, elliptical-like structure. It has a concentrated central bulge that is yellow, indicating an older stellar population. The overall shape is primarily round, with a slight elongation that can barely be identified. There are no spiral arms or dust lanes visible. There is some mild, minor irregularities in the outer regions indicating that the galaxy may have had some disturbances, and that the galaxy is likely undergoing a low amount of star formation. Overall, it appears to be an intermediate mass galaxy.
