The galaxy appears as a somewhat smooth, elliptical-like structure with a concentrated central bulge. The light distribution is centrally peaked, with the highest intensity emanating from the core. The overall color is generally yellow/orange indicating an older stellar population. There is faint evidence of a very subtle disk component, but it is not prominent. The outer regions of the galaxy are more diffuse, fading gradually into the background. Faint disturbances might be present, suggesting the possibility of minor gravitational interactions or past merger events, however, the galaxy is primarily undisturbed.
