The galaxy presents a generally smooth and elliptical morphology, appearing largely featureless at this resolution. It is centrally concentrated, exhibiting a bright, yellowish core that gradually fades into a more diffuse halo. The overall color suggests an older stellar population. There is no evidence of prominent spiral arms or a significant disk component. Subtle color variations hint at possible underlying structure, though it appears primarily quiescent. The rounded shape and lack of strong disturbances indicate a relatively relaxed state, potentially indicative of a more evolved system.
