The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The core exhibits a bright, yellowish-white hue suggestive of an older stellar population. This area transitions outward to a bluer, less concentrated halo. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy appears relatively undisturbed with no obvious signs of major mergers or tidal features, although there may be minor irregularities in the outer regions of the halo. The overall round shape indicates a minimal degree of rotational support. This galaxy likely has a significant stellar mass and relatively low ongoing star formation.
