The galaxy presents as a luminous, centrally concentrated elliptical system, exhibiting a smooth morphology with no apparent spiral arm structure or significant dust lane obscuration. Its overall color is consistent with an older stellar population, with a slight bluing near the edges. The system displays a high degree of rotational symmetry, leaning towards a circular shape. There is no visual evidence of ongoing major mergers or significant tidal disturbances, although subtle minor disturbances cannot be ruled out. 
