The galaxy presents as an elliptical structure, exhibiting a smooth, concentrated light profile with a slight elongation. A prominent central bulge is visible, characterized by a yellowish-orange hue indicative of an older stellar population. Fainter, diffuse outer regions suggest a gradual decline in stellar density with increasing radial distance from the core. Overall, the galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions.
