The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a bright, concentrated central bulge that appears to be the dominant feature. The light profile diffuses outward from this bright center, gradually fading into the background sky. There is a hint of a disk-like structure, but it is subtle and poorly defined. The galaxy does not display any prominent spiral arms or significant dust lanes. The overall color is consistent with an older stellar population. There is no evidence of any major ongoing mergers or significant tidal disturbances. The object is likely a large, relatively massive galaxy with minimal current star formation activity.
