The galaxy presents as an elliptical morphology with a smooth light profile and no apparent disk structure. Its color index suggests a population of older stars, with a central bright region that could be a core of concentrated stars, or possibly an active galactic nucleus. No spiral arm structures are visible. The overall appearance is consistent with a galaxy that has undergone substantial evolutionary aging, and minimal star formation. There is no evidence of tidal interactions or disturbances, supporting the finding that it is a relatively undisturbed galaxy.