The galaxy presents as a centrally concentrated object with a smooth, diffuse light distribution, characteristic of an elliptical morphology. It exhibits a slightly elongated shape. The core region appears bright and yellowish-white. There is a subtle color gradient from the core outwards, trending toward a slightly redder hue in the outer regions. No distinct spiral arms or dust lanes are discernible within the limitations of this image. There are no obvious signs of a major ongoing merger event, though subtle irregularities in the outer halo cannot be ruled out. The overall structure suggests a relatively evolved system with a substantial spheroidal component and a moderate level of star formation activity.
