The galaxy presents a largely smooth and elliptical morphology, exhibiting a moderate elongation. The light profile appears centrally concentrated, characterized by a bright, yellowish core that gradually fades into the surrounding halo. The galaxy exhibits a noticeable color gradient, transitioning from a warmer, more luminous central region to cooler, fainter peripheries. There is no visual evidence of spiral arms or significant dust lanes; the galaxy appears relatively undisturbed, with only slight asymmetries hinting at minor disturbances. The overall impression is that of a relatively massive galaxy with a low star-formation rate.
