The galaxy presents as a smooth, centrally concentrated object, likely an elliptical galaxy, based on its morphology. Its core exhibits a bright, yellow-white luminosity, suggesting a population of older stars dominating the central region. The galaxy appears nearly spherical, with a high degree of roundness. There is no discernible spiral arm structure or significant dust lane obscuration visible. The galaxy's periphery shows a gradual decrease in surface brightness, transitioning to the background sky. There is no strong evidence of ongoing or recent major mergers or tidal disturbances in the immediate vicinity, and the system appears relatively isolated and undisturbed. Overall, the galaxy seems like a well-established, relatively quiescent system, with an apparently low rate of current star formation.
