The galaxy presents a roughly circular morphology. The light distribution appears centrally concentrated with a smooth, diffuse halo extending outwards. The central region exhibits a brighter, slightly elongated core. There are some subtle color gradients, with the core exhibiting a slightly redder hue compared to the bluer outer halo. There is no clear indication of spiral arm structure or a prominent disk, suggesting a relatively smooth distribution of stars. Overall, the galaxy appears to be an elliptical type with a dominant bulge component and a lack of significant recent merger activity. Based on the subtle red color of the core and the blue outer halo, there might be ongoing star formation activity, but the current rate is probably moderate. There is a slight asymmetry in the diffuse halo which could indicate a minor gravitational interaction with a satellite galaxy that is not visible.
