The galaxy presents as a generally smooth, elliptical object. The central region exhibits a high surface brightness, appearing concentrated and spheroidal. A gradual decrease in luminosity is observed moving outward from the core. The galaxy appears relatively undisturbed, lacking prominent spiral arms or tidal features indicative of recent major mergers. Faint, subtle asymmetries may be present in the outer regions, potentially suggesting minor disturbances or past interactions. The galaxy appears to be a yellow hue, which could indicate an older stellar population.
