The galaxy presents an elliptical morphology, appearing elongated in shape. There is a smooth, centrally concentrated brightness profile, suggesting a relatively old stellar population. The galaxy exhibits a subtle color gradient, with the central region appearing slightly bluer than the outer regions, which could indicate some ongoing star formation. No distinct spiral arms or prominent dust lanes are visible. The overall structure implies it is likely an early-type galaxy undergoing some level of star formation. There are no signs of any ongoing mergers or tidal disturbances.
