The galaxy presents a largely smooth, elliptical morphology. It is a relatively compact object with a concentrated central bulge that exhibits a yellow-orange hue, suggestive of an older stellar population. A faint, diffuse halo surrounds the core region, transitioning to a bluer color as it extends outward. This subtle color gradient implies the presence of younger stars or ongoing star formation in the galaxy's outer regions, though the rate appears to be low. There is no evidence of strong spiral arm structures or significant morphological disturbances, and the overall appearance is generally undisturbed. 
