The galaxy presents a generally smooth, elliptical morphology. The central bulge appears bright and concentrated, transitioning to a fainter, more diffuse halo. Color gradients indicate that the core regions are yellower, suggestive of an older stellar population, while the outer regions are slightly bluer, which could indicate some presence of younger stars, though at a very low rate. The overall shape is not perfectly circular, exhibiting a slight elongation which does not resemble a clear disk structure. There is no evidence of any significant tidal features, spiral arms, or strong disturbances to its morphology; the galaxy seems relatively undisturbed. Close inspection reveals that there are no obvious signs of a major ongoing merger event. Though subtle asymmetries are noted, these do not strongly suggest a recent interaction.
