The galaxy presents as a somewhat elongated, lenticular or possibly elliptical-type galaxy. Its core exhibits a concentrated, bright, yellowish-white hue, suggesting a significant population of older stars. There appears to be a smooth transition from the core outward. The outer regions of the galaxy display a more diffuse, fainter glow compared to the central core. There is no distinct presence of spiral arms or significant dust lanes visible in the image. Overall, the galaxy appears relatively undisturbed, without major signs of ongoing mergers or tidal interactions.
