This galaxy exhibits a smooth, elliptical morphology. It presents a concentrated central bulge that dominates its overall structure, with a significant decrease in luminosity moving outwards from the center. The color profile suggests the bulge consists of older stellar populations. A disk can be seen around the bulge, which appears to be more blue, indicating possible star formation. The galaxy does not appear to be undergoing a major merger event, however, there is evidence of minor disturbance. The lack of strong spiral arm structures points towards a classification as either an elliptical galaxy or a lenticular galaxy with a significant bulge component.
