The galaxy presents as a smooth, elliptical-like structure. Its core exhibits a concentrated, yellowish-orange hue, suggesting a population of older stars, or perhaps significant dust obscuration. The outer regions transition to a more diffuse, greenish-blue tint, possibly indicating the presence of a younger stellar population, or regions of ongoing star formation. Overall, the galaxy appears relatively undisturbed, displaying no obvious signs of tidal interactions or major mergers. A slight asymmetry is observed, but does not suggest any recent disturbance, merger, or interaction. 
