The galaxy presents as a relatively smooth, elliptical structure with a notable central bulge. Its overall shape appears elongated, with a clear major axis and a shorter minor axis. There is a slight color gradient visible, with the core exhibiting a yellowish-white hue, potentially indicating a population of older stars. The outer regions appear slightly bluer, suggesting some presence of younger stars or ongoing star formation, though this is not very prominent. There is no readily apparent spiral arm structure or significant dust lane features visible in this imaging. The galaxy appears relatively undisturbed with no obvious signs of a recent major merger event.
