The galaxy presents as a centrally concentrated object, appearing largely smooth and elliptical in shape. There is minimal evidence of spiral arms or significant disk features. The color gradient suggests a yellowish-orange core, possibly indicating an older stellar population dominating the central region. Fainter, diffuse greenish hues extend outward from the core, potentially representing regions of more recent, though subdued, star formation. The overall morphology suggests a galaxy that is relatively evolved, with little evidence of recent major mergers or significant disturbances.
