This galaxy exhibits a generally smooth, elliptical morphology. It displays a prominent central bulge, which appears to be the dominant feature. The galaxy appears to be observed at a high inclination, potentially edge-on. There are no clear signs of spiral arm structure or a significant disk component visible in this image, but there is some minor disturbance. Evidence of a weak bar could be present. There are no apparent major merging signatures, though a minor disturbance cannot be ruled out. Color gradients suggest older stellar populations are concentrated in the central regions, with bluer, possibly younger populations extending into the outer halo.
