The galaxy presents as a concentrated, luminous core, transitioning to a broader, less defined outer region. The overall form appears largely elliptical, displaying a high degree of circularity. Little to no disklike structure or spiral arm features are discernible in this image. Coloration indicates a mature stellar population, particularly within the core, which displays a distinct reddish-yellow hue. There is a subtle suggestion of bluer colors at the peripheries, implying the existence of some younger stars, but overall, there is a low amount of star formation, if any at all. There is no evidence of recent or ongoing major mergers. The galaxy appears relatively undisturbed. The distribution of light is fairly smooth and centrally concentrated.
