The galaxy appears as a centrally concentrated, smooth object, with a relatively elliptical shape. There is no obvious presence of spiral arms or a prominent disk structure. The galaxy exhibits a smooth and diffuse light distribution across its body. The galaxy's core appears bright and concentrated. The light profile suggests that it is likely an early-type galaxy. There is no substantial evidence of ongoing merging activity or major disturbances in its morphology. The overall color gradient seems blueish, which could indicate some recent star formation, even though the dominant population appears to be older stars based on its smooth appearance.
