The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a noticeable color gradient, transitioning from a yellowish-white core to a bluer outer halo. The core exhibits a high degree of luminosity, suggesting a significant population of older stars. The overall structure appears relatively undisturbed, with no obvious signs of tidal tails or major distortions indicative of recent mergers. The color and morphology imply that the galaxy is relatively massive, with a moderate star formation rate.
