The galaxy presents as a centrally concentrated object with a smooth overall morphology. It exhibits an elliptical shape with a relatively high degree of central light concentration, fading outwards. Color gradients are subtle, with a slightly redder core possibly indicating an older stellar population compared to the surrounding regions. The light distribution suggests a relatively high Sersic index, indicative of an elliptical galaxy. The galaxy appears undisturbed, showing no major signs of tidal interactions or ongoing mergers. A slight asymmetry can be seen.
