The galaxy presents as a smooth, elliptical-like structure. Its color profile exhibits a yellowish-orange hue, suggesting a population of older stars and a relatively low rate of ongoing star formation. The morphology appears largely undisturbed, with no significant signs of tidal interactions or major mergers. The galaxy exhibits a high degree of roundness. The overall appearance indicates a passively evolving system likely dominated by an older stellar population, and high mass. 
