The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal. The central region exhibits a high surface brightness, indicative of a concentrated stellar population. The color gradient shows a shift toward redder hues in the core. Fainter, diffuse light extends outward from the center, forming a halo with a less distinct boundary. There appears to be a very minor asymmetry or disturbance in the halo region, with a slight extension on one side of the galaxy, but is not conclusive.
