The galaxy presents a flattened, elongated morphology, appearing as a prolate spheroid with a high axis ratio. Its overall color index indicates a significant population of older stars, particularly concentrated in the central bulge, which exhibits a reddish hue. Fainter blue-ish regions are visible at the edges.

There is no clear evidence of spiral arm structure. Additionally, the image suggests only a very minor gravitational disturbance or interaction with other objects in its immediate vicinity. Overall, the galaxy appears relatively undisturbed and exhibits a smooth morphology, consistent with that of an elliptical galaxy.
