The galaxy presents as a centrally concentrated, smooth elliptical morphology. The core exhibits a bright, yellowish-white color, indicating an older stellar population. There is a gradual decrease in luminosity moving outward from the core, transitioning to a fainter, redder halo. The shape appears largely spheroidal, with a slight deviation from perfect circularity. There is no clear indication of spiral arms or a prominent disk structure. The overall structure is relatively undisturbed, with no obvious signs of ongoing major merger events.
