The observed galaxy exhibits a generally smooth morphology, with an elliptical, elongated shape. The galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal disruptions. The light distribution is centrally concentrated, displaying a bright, yellowish core, which suggests an older stellar population dominating the central region. The outer regions of the galaxy gradually fade into a more diffuse halo, showing hints of bluer colors, potentially indicating the presence of younger stars and some ongoing, though likely subdued, star formation. Overall, it appears to be a quiescent galaxy with a substantial bulge component.
