The galaxy exhibits a smooth, elliptical morphology. It is elongated in shape, appearing cigar-shaped. The light distribution indicates a concentration of older stellar populations towards the central regions, which display a yellowish hue. Fainter, bluer components can be seen toward the outer edges of the galaxy. The galaxy appears to be relatively undisturbed, showing no significant signs of ongoing or recent major merger activity. The disk component seems to be more prominent than distinct features, which are more difficult to discern. Overall, the galaxy appears to be a relatively evolved system with a significant spheroidal component.
