The galaxy presents as a resolved object with a noticeable elliptical morphology. It exhibits a smooth and concentrated central region, characteristic of an elliptical galaxy. The radial light profile appears to decrease smoothly from the center outwards, with no distinct spiral arms or significant dust lanes visible. The color index suggests a population of older stars, as indicated by its redder hue. There are no apparent signs of major recent mergers or tidal disturbances. The galaxy exhibits a moderate axial ratio, appearing somewhat elongated.
