The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a generally elliptical morphology, with a high degree of roundness. A bright, yellowish core region dominates the galaxy's luminosity profile, suggesting an older stellar population concentrated towards the center. The color gradient transitions from a yellowish core to a slightly bluer halo, indicating the presence of younger stars in the outer regions, although the overall color suggests a galaxy dominated by an older population. There are no obvious signs of spiral arms or a prominent disk structure. The galaxy appears relatively undisturbed, showing no major signs of tidal interactions or ongoing mergers, although subtle asymmetries may be present that could suggest minor disturbances. Overall, it presents as a fairly evolved system with a smooth morphology.
