The galaxy presents a generally smooth, elliptical morphology. Its light profile increases towards the center, suggesting a centrally concentrated stellar population. There is no clear evidence of spiral arms or a prominent disk structure. The object exhibits a roughly circular shape and the color appears generally uniform across the galaxy, though the central region displays a yellowish hue, possibly indicative of older stars. Overall, the galaxy appears relatively undisturbed, with no significant signs of a recent major merger. Faint extended light is visible suggesting a stellar halo.