The galaxy exhibits a flattened, elliptical morphology. The central region appears brighter and more concentrated, possibly indicating a bulge component. The outer regions appear fainter and more diffuse, suggesting a disk-like structure. There are no clear spiral arm features visible; the galaxy seems largely smooth. The galaxy possesses a generally blue hue, particularly within its central and disk regions, which suggests ongoing or recent star formation. There may be signs of minor disturbances or asymmetries in the galaxy's structure, which could be due to tidal interactions or recent minor merger activity. The overall shape and appearance suggests that this galaxy is most likely an intermediate spiral galaxy, though it may be an elliptical galaxy experiencing star formation.
