The galaxy presents as a centrally concentrated, elliptical morphology. It exhibits a smooth, largely featureless structure with a high degree of rotational symmetry. The color profile indicates a population of older stars, shifting from a red core to a slightly bluer but still yellowish halo. There is no obvious evidence of spiral arms or active star formation regions visible in this image, and no significant tidal disturbances or signs of mergers can be identified. The galaxy presents as a fairly regular spheroid.