The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually diffuses outward into a fainter halo. There is no clear evidence of spiral arm structure or a prominent disk. The color profile appears relatively uniform across the galaxy, with a slight reddening toward the central bulge, possibly indicating an older stellar population in that region. There is no obvious sign of tidal features or recent mergers, and the overall structure seems undisturbed.
