The galaxy presents a generally smooth, elliptical morphology. Its light profile appears relatively uniform, with no discernible spiral arms or prominent dust lanes. The central region appears slightly brighter than the outer regions, suggesting a possible concentration of stars toward the galactic nucleus. The overall color of the galaxy is moderately red, which implies an older stellar population. The galaxy seems to be relatively undisturbed, showing no obvious signs of recent mergers or tidal interactions.
