The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated, centrally-brightened core, indicative of a likely bulge component. The overall shape is quite rounded, with only slight deviations from a perfect circle. Faint color variations are visible; the central region appears to exhibit a yellower hue, possibly indicating an older stellar population, while the outer regions have a slightly bluer tint, perhaps signaling the presence of younger stars or ongoing star formation, though at a low rate. There is no visible evidence of major disturbances, tidal features, or ongoing mergers.
