The galaxy presents as a largely smooth, centrally concentrated object. Its morphology appears primarily elliptical. The light distribution exhibits a high degree of radial symmetry, with a gradual decrease in surface brightness from the core outwards.

A color gradient is observed. The central region has a yellow-white hue, transitioning to a more blue-ish color in the outer regions. This suggests a potential age gradient in the stellar population, with older, redder stars dominating the core and younger, bluer stars contributing more significantly to the outer halo. There is no evidence of spiral arms or a distinct disk structure. Some slight irregular structure at the edges may indicate very minor disturbances. 
