The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-orange, possibly indicative of an older stellar population. The light distribution appears fairly uniform and radially symmetric. There's a gradual decrease in luminosity moving outwards from the central bulge into a diffuse halo. There are no apparent spiral arms or significant dust lanes visible. The overall structure suggests the galaxy is a relatively undisturbed system with no obvious signs of recent major mergers or tidal interactions, although some minor disturbances cannot be ruled out.
