The galaxy exhibits a generally smooth morphology, with a bright, centrally concentrated core. There is evidence of a more extended, diffuse halo surrounding the core. Color gradients are noticeable; the central region appears redder, transitioning to a more greenish hue in the outer regions of the halo. The overall shape seems slightly elongated, but predominantly rounded. There are no obvious signs of strong tidal interactions or major disturbances in its structure, although some minor asymmetries may be present in the halo. The galaxy does not appear to possess a prominent disk structure.
