The galaxy appears to be a relatively smooth, elliptical-type galaxy. It is somewhat rounded in shape, but not perfectly spherical. There is a concentration of light towards the center, suggesting a dense galactic nucleus. The galaxy exhibits a gradual decrease in brightness as you move outward from the center, implying a diffuse halo. There are no obvious spiral arms or strong dust lanes visible. The overall color of the galaxy is slightly blueish, indicating a small amount of recent star formation activity and suggesting a likely relatively old stellar population. There is no indication of major mergers or significant tidal disturbances. The galaxy is well-defined and appears isolated.
