The galaxy presents an elliptical morphology, appearing as a smooth, centrally concentrated structure. A bright, yellowish core dominates the visual appearance, suggesting a significant population of older stars. There is a subtle color gradient visible, with the central region appearing yellower compared to the outer regions. This color difference may indicate variations in stellar population or dust content. The outer regions of the galaxy exhibit a faint, diffuse halo. There is some minor asymmetry present, possibly indicating a past interaction or disturbance, though there is no clear evidence of an ongoing merger. The galaxy's overall smooth appearance suggests it is a relatively evolved system.
