The galaxy presents as a moderately bright, elliptical system with a smooth, centrally concentrated light profile. The core region exhibits a yellowish-white hue, suggesting an older stellar population and a likely absence of significant ongoing star formation in that area. Moving outward from the center, the galaxy fades into a slightly bluer halo, possibly indicating the presence of a younger, though still relatively quiescent, population of stars. The galaxy appears to be relatively undisturbed, displaying a regular and symmetrical morphology with no signs of major mergers or tidal interactions. The overall shape is slightly flattened, deviating marginally from a perfect circle. The light distribution suggests a Sersic index typical of elliptical galaxies.
