The galaxy presents as a relatively smooth, elliptical structure. Its overall color is a yellowish-white, suggesting a population of older stars with lower recent star formation activity. The core of the galaxy appears slightly brighter than the surrounding regions, indicative of a possible concentration of stars towards the center. There is faint evidence of a disk. The general morphology suggests a galaxy that has undergone significant evolution and likely has a substantial mass. It appears to be relatively isolated, without any clear signs of major mergers or significant tidal disturbances.
