The galaxy presents as a largely smooth, elliptical or lenticular structure. There is a prominent central bulge which appears a yellowish-white hue, suggesting a population of older stars. The galaxy displays a relatively high degree of symmetry. The outer regions exhibit a gradual decrease in luminosity, transitioning from a yellow hue nearest the center to what appears to be a reddish-orange color further from the nucleus. There is a lack of prominent spiral arm structures or dust lanes. There is no clear evidence of ongoing major mergers or significant tidal distortions. The overall morphology suggests a relatively evolved system.
