The galaxy presents as a smooth, centrally concentrated object, displaying an elliptical morphology. The light distribution suggests a dominant bulge component, appearing roughly rounded but elongated. The core exhibits a reddish hue, potentially indicating a population of older stars or significant dust obscuration. A faint greenish glow surrounds the core, extending outward. This emission could arise from younger stellar populations undergoing active star formation. There are no obvious signs of strong tidal disturbances or major mergers. The overall appearance suggests a relatively quiescent system.
