The galaxy presents as a centrally concentrated, elliptical morphology with a smooth light distribution. A discernible central bulge exhibits a yellowish-white hue, suggesting a population of older, evolved stars. The outer regions of the galaxy transition to a fainter, less-defined halo, which appears slightly bluer than the core, potentially indicating the presence of a younger stellar population or a small amount of ongoing star formation. The galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions. Overall, the galaxy is likely a massive system.
