The galaxy presents as a diffuse, elliptical-shaped object. It exhibits a smooth, centrally concentrated morphology with a noticeable color gradient, transitioning from a yellowish-orange core to fainter, bluer outer regions. The galaxy appears elongated, suggesting a possible classification as an elliptical galaxy of type E4 or E5. There is no visible evidence of spiral arms, dust lanes, or active star formation regions, suggesting that star formation has largely ceased within the galaxy. There might be very minor tidal disturbances if the galaxy is undergoing a minor merger event, or have undergone one recently. The overall structure indicates a well-evolved system dominated by an older stellar population.
