The galaxy presents as a luminous, centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, suggesting a population of older, evolved stars. There is a subtle color gradient extending outward from the core, transitioning to a slightly greener tinge in the outer regions. This subtle green may be due to the presence of younger stars beginning to form in those regions. The galaxy appears largely undisturbed, showing no prominent signs of tidal interactions or ongoing major mergers. It lacks a distinct disk structure or spiral arms, further supporting its classification as an elliptical galaxy. Overall the galaxy appears rounded with no signs of disturbance.