The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. The core exhibits a strong yellow-orange hue, suggesting a significant population of older stars. Progressing outward, the galaxy transitions to a more diffuse, greenish-blue color, possibly indicative of ongoing, albeit subdued, star formation in the outer regions. There is no discernable spiral structure. The overall appearance indicates a system that is relatively undisturbed, lacking any major signs of tidal interactions or ongoing mergers, with the majority of its stars being quite old.
