The galaxy appears to be an elliptical or lenticular galaxy. It has a smooth, diffuse light distribution, with a centrally concentrated bulge. There is no evidence of spiral arms or significant dust lanes. The galaxy exhibits a yellowish hue, suggesting a population of older stars, with relatively little ongoing star formation. The overall morphology is relatively undisturbed, showing no signs of major mergers or tidal interactions. There might be some slight indications of minor disturbances, however the smoothness of the light profile suggest the system is nearing a stable state. The light appears roughly symmetrical and round, with no apparent elongations or asymmetry.
