The galaxy presents as a diffuse, centrally concentrated structure. It appears to have an elliptical morphology with a smooth texture, lacking prominent spiral arms or other distinct features. The core region exhibits a brighter, more luminous appearance, indicative of a higher stellar density. The outer regions gradually fade into the background sky, suggesting a decreasing stellar population density with increasing radial distance from the galactic center. The overall color is a pale blue. There is little to no evidence of significant dust lanes or ongoing major star formation activity discernible in the image. The galaxy appears to be relatively undisturbed, showing no signs of major mergers or tidal interactions.
