The galaxy presents an elongated, elliptical morphology, with a distinct central bulge that appears relatively smooth and concentrated. A fainter, extended disk surrounds the bulge, displaying a bluish hue that could indicate the presence of younger stellar populations and ongoing star formation. The disk appears somewhat disturbed or irregular, possibly due to interactions or internal dynamics. The overall structure suggests a spiral galaxy seen at a significant inclination, obscuring a clear view of any spiral arm structure. There is also the potential of a minor merger to the left of the central bulge, though the resolution makes that difficult to discern. 
