The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a yellowish-orange hue, suggesting an older stellar population. A diffuse, greenish-blue halo surrounds this central bulge, indicating the presence of some younger, bluer stars, although the overall star formation rate appears to be low. The galaxy exhibits a mostly undisturbed structure, showing no signs of major mergers or significant tidal disruptions. It possesses a notably large mass and relatively compact size.
