The galaxy presents as a centrally concentrated, generally smooth, and elliptical-appearing structure. It exhibits a noticeable color gradient, transitioning from a bright, yellowish core to a more diffuse, blue-tinged outer region. There are no discernible spiral arms or bar structures. The galaxy appears largely undisturbed, showing no major signs of tidal interactions or recent mergers. The observed morphology suggests a system dominated by older stellar populations, particularly in the central regions, with some evidence of ongoing, albeit subdued, star formation in the outskirts. The roundness of the galaxy is high with only slight deviations away from being perfectly circular.
