The galaxy exhibits a centrally concentrated luminosity profile, appearing smooth and elliptical in shape. The core is a bright, nearly uniform yellow-white hue, suggesting an older stellar population and minimal ongoing star formation in the nuclear region. A fainter, more diffuse halo surrounds the core, displaying a subtle color gradient from yellow-white to a slightly redder shade as the radius increases. The ellipticity of the galaxy is moderate, and the overall structure indicates it is unlikely to be a spiral galaxy. There are no visually apparent signs of mergers or significant tidal disturbances.
