The galaxy appears to be a relatively bright, smooth, elliptical galaxy. It exhibits a concentrated central bulge that emits strongly, with color suggesting an older stellar population. The overall shape is somewhat ellipsoidal, appearing neither perfectly spherical nor highly elongated. There is a gradual decrease in brightness moving from the core outwards, with minimal evidence of spiral arms or significant disk features. Faint extensions surround the main body of the galaxy. There is no obvious sign of any strong tidal disturbances or ongoing merging activity.
