The galaxy presents as a generally elliptical morphology with a smooth, concentrated central bulge. There is a subtle color gradient observable, with the central regions exhibiting a yellowish hue, potentially indicative of an older stellar population. The outer regions appear slightly bluer, suggesting the presence of some younger stars, but this is subtle. There is no discernible spiral arm structure or significant dust lane presence. The overall structure indicates the galaxy is relatively undisturbed, with no major signs of tidal interactions or ongoing mergers.
