The galaxy presents as an elliptical or lenticular system with a smooth, diffuse light distribution. Its overall color appears to be an average of colors. The central region shows a concentration of light, suggesting a possible galactic bulge or core. The light tapers off gradually with increasing radius, with no discernible spiral arms or distinct disk-like features are visible. The structure appears largely undisturbed, lacking any obvious signs of recent mergers or tidal interactions. The roundness of the galaxy indicates an elliptical morphology.
