The galaxy presents as a relatively smooth, elliptical structure. There is a concentrated central bulge that appears bright yellow, indicative of an older stellar population. Moving outward from the core, the galaxy exhibits a gradual decrease in luminosity. The overall shape is noticeably elliptical, with the major axis longer than the minor axis. There is little evidence of spiral arms or significant dust lanes. Some minor disturbance or interaction is possible based on the outer edges of the galactic halo.
