The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a noticeable gradient in luminosity, with the core region significantly brighter and more intensely colored than the surrounding halo. The color profile suggests an older stellar population, with a pronounced red-yellow hue in the central regions. The outer edges of the galaxy gradually fade into the background, exhibiting a subtle transition. The overall morphology indicates a system that has undergone significant dynamical relaxation, with minimal evidence of spiral arms or active star formation regions based on the color and smoothness of the light distribution. It appears mostly undisturbed without signs of major recent merger activity, although some minor asymmetry cannot be ruled out.
