The galaxy presents as a largely homogenous elliptical form with a central concentration of luminosity. The core region exhibits a yellowish-white hue, suggestive of an older stellar population, while the outer halo displays a bluer tint, potentially indicating the presence of younger stars or ongoing, albeit limited, star formation. The overall morphology appears relatively undisturbed, lacking any prominent tidal features or asymmetries indicative of recent major mergers or significant gravitational interactions. The shape approximates a rounded form, leaning towards a slightly elliptical profile rather than a highly elongated or cigar-shaped appearance. There is no indication of a central bar or spiral arm structure. The smooth appearance is consistent with a galaxy where a significant fraction of the interstellar medium has been depleted.
