The galaxy presents as a centrally concentrated, relatively smooth object. Its light profile appears to be largely elliptical, displaying a high degree of radial symmetry. A slight elongation can be discerned, though the axial ratio is close to unity. The color gradient suggests a redder core, transitioning to slightly bluer hues in the outer regions, possibly indicative of differing stellar populations or dust distribution. There are no obvious spiral arm structures or prominent dust lanes visible. The overall morphology appears undisturbed, with no clear signs of recent mergers or major interactions, though a very slight asymmetry might indicate a minor disturbance. The galaxy displays a moderate degree of brightness.
