The galaxy presents as a somewhat elliptical structure with a smooth, diffuse morphology. It is dominated by a bright, yellowish central bulge region, indicative of a relatively older stellar population. The outer regions exhibit a bluer hue, possibly suggesting the presence of younger stars or ongoing star formation. There is a subtle hint of a disk-like structure, though it is not sharply defined. Overall, the galaxy appears to be relatively undisturbed, showing no significant signs of recent major mergers or tidal interactions.
