The galaxy presents as a relatively smooth, elliptical morphology. Its light profile appears concentrated toward the center, indicating a prominent bulge component. Color gradients are subtle, with a slight reddening toward the core, potentially indicative of an older stellar population dominating the central regions. The overall shape suggests a relatively low degree of rotational support. There is no evidence of strong spiral arm structure or active star-forming regions visible in this image. The color suggest moderate to high mass galaxy with a low star forming rate. There are hints of minor tidal features or disturbances, but no strong indication of a major ongoing merger event. Overall, the galaxy appears to be a relatively quiescent elliptical or lenticular galaxy.
