The galaxy presents a primarily smooth and elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-white, suggesting a high density of older stellar populations. The outer regions display a gradual decrease in brightness, fading into the background. The overall shape is elongated, with a suggestion of a prolate spheroid. There is no strong evidence of spiral arms or significant dust lanes. The smoothness and colour suggest that the galaxy is potentially undergoing little current star formation. There is a slight asymmetry, potentially a minor gravitational disturbance or faint tidal features may be present in the outer regions, indicating a possible past interaction or minor merger event.
