The galaxy presents an elliptical morphology, displaying a smooth, diffuse light distribution. The light appears centrally concentrated, exhibiting a brighter, yellowish core. The outer regions gradually fade into the background sky, showing a bluer hue than the core. There is no obvious spiral arm structure or dust lane features visible. Based on the smooth light distribution, the galaxy appears to be relatively undisturbed, with no major signs of ongoing mergers or tidal interactions.
