The galaxy appears as a generally smooth, centrally concentrated object. Its morphology suggests a large, early-type system, potentially an elliptical galaxy or a lenticular galaxy with a prominent bulge. The color profile indicates a redder core, transitioning to slightly bluer outer regions, suggesting a population of older stars in the center with some younger stars possibly present in the outer areas. There are no obvious spiral arm structures or significant dust lanes visible, and the overall appearance seems relatively undisturbed. The shape is largely round. There is no evidence of a major merger event in its recent past, with the overall structure appearing largely relaxed and evolved. 
