The galaxy presents as a centrally concentrated, relatively smooth structure. Its overall shape is approximately circular, indicating a lack of significant angular momentum or recent major merger events. The core region exhibits a bright, yellowish-white luminosity, suggesting a population of older stars and/or significant dust obscuration. There is a subtle color gradient outwards from the core, transitioning toward a slightly bluer hue in the outer regions. This implies the presence of some younger stellar populations in the surrounding regions, though the overall star formation rate appears to be relatively low. No distinct spiral arms or bar structures are apparent in the visible light bands. There is no evidence of strong tidal tails or other morphological disturbances that would indicate ongoing or recent merger activity, though there may be minor disturbances present. Overall, the galaxy appears to be an early-type galaxy transitioning toward a more passive state.
