This galaxy appears to be a relatively smooth, centrally concentrated system, most likely an elliptical galaxy. It exhibits a somewhat spheroidal morphology with no obvious spiral arm structure or prominent dust lanes visible. The galaxy displays a bright central bulge, which seems to gradually fade into an outer halo. There is some color variation, with the central region appearing more yellow, possibly indicating an older stellar population, and the outer regions display bluer hues, which may indicate the presence of younger, hotter stars. Overall, the galaxy appears to be relatively undisturbed, with no indications of major mergers or tidal interactions.
