This galaxy presents as a generally smooth object, with a slightly elongated, elliptical morphology. The light is concentrated toward the center, exhibiting a bright, yellowish core, indicating an older stellar population likely dominates the central region. Moving outward from the core, the light gradually diffuses into a more extended, fainter halo. The outer regions appear slightly bluer in color relative to the core, suggesting the presence of a younger population of stars or ongoing star formation. There is no obvious evidence of strong spiral arm structure or major mergers, although minor disturbances or subtle tidal features cannot be entirely ruled out. The overall appearance is consistent with a massive galaxy at a significant redshift.
