The galaxy presents as a centrally concentrated object with an overall elliptical morphology. The core exhibits a yellowish-white hue, suggesting a population of older stars. A diffuse, bluer halo surrounds the core region, indicating the presence of younger stellar populations and potential star formation activity. The galaxy appears relatively undisturbed, with no obvious signs of tidal features or ongoing major mergers. However, some subtle irregularities in the outer halo might suggest minor interactions or disturbances. The overall smoothness of the light distribution is interrupted by some patches of more distinct structures, such as possible faint spiral arms or dust lanes. The axial ratio suggests that the galaxy is not viewed perfectly face-on, but exhibits a moderate inclination angle.
