The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution suggests a dominant spheroidal component. There appears to be a slight deviation from perfect circularity. Color gradients are subtle, with the central region appearing somewhat bluer compared to the outer regions. There are no obvious spiral arms, bars, or other distinct features indicative of a disk galaxy. There may be some minor disturbances. Based on its morphology, the galaxy is likely an elliptical or S0 type.