The galaxy appears to be a relatively smooth, centrally concentrated system, likely an elliptical or lenticular type. It exhibits a moderate ellipticity, appearing slightly rounded rather than highly elongated. The light profile suggests a bulge component dominating the overall structure, with a gradual decrease in intensity moving outward from the core. There is a faint blue tinge to the outer regions, suggesting some ongoing, though limited, star formation. No distinct spiral arms or strong dust lanes are visible. There are no obvious signs of recent major merger activity, although a slight asymmetry in the outer isophotes could indicate a past minor interaction. The central region appears to be quite luminous, possibly indicating the presence of an active galactic nucleus, or a high density of stars. Overall, the galaxy presents a quiescent, evolved morphology.
