The galaxy presents as a relatively smooth, elliptical-like object. It displays a concentrated central bulge, with a gradual decrease in luminosity towards its outer regions. The core exhibits a yellowish hue, suggestive of an older stellar population. The outer regions show hints of bluer colors, indicating the presence of younger, hotter stars, although these features are not strongly pronounced. There is a noticeable lack of distinct spiral arms or prominent dust lanes. The overall morphology suggests a system that has undergone significant dynamical relaxation, with a high degree of symmetry. There is no evidence of a major ongoing merger event.
