The galaxy presents as a centrally concentrated object with a relatively smooth appearance, lacking distinct spiral arm structures or a prominent disk. It exhibits a generally elliptical shape, appearing nearly circular. The light distribution suggests a fairly homogenous stellar population, with the core showing a slight increase in luminosity. Overall, the galaxy appears to be relatively undisturbed, without any obvious signs of major mergers or tidal interactions. Subtle color variations are present, but they are not particularly pronounced, indicating a moderate range in stellar ages and metallicities. The blue light is more dominant in the center of the galaxy.
