The galaxy presents as an elliptical structure with a smooth appearance, suggesting an older stellar population. It exhibits a notable central bulge, which is elongated in shape. The color gradient transitions from a yellowish core to slightly redder outer regions, indicative of a potentially dusty environment or varying age of stellar populations within the galaxy. While the galaxy appears relatively undisturbed, subtle asymmetries in its outer regions might indicate past minor interactions, though no clear merger events are immediately apparent.
