This galaxy presents as a bright, centrally concentrated elliptical structure with a high degree of smoothness. The light distribution suggests a bulge-dominated system, with a relatively small disk component observed nearly edge-on. The color profile appears slightly redder in the central regions, possibly indicating an older stellar population. There are subtle features of asymmetry or minor disturbances present within the galaxy's outer regions. The galaxy exhibits a slightly elongated shape, indicating a deviation from perfect circularity. Overall, the morphology points towards a galaxy that has likely undergone significant dynamical evolution and star formation quenching.