The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears primarily spheroidal, exhibiting a high degree of circularity. There is little discernible internal structure such as spiral arms or a prominent disk. The galaxy displays a color gradient, with a bluer, brighter central region transitioning to a redder, fainter outer halo. There are no obvious signs of major disturbances or ongoing mergers. Minor irregularities cannot be completely ruled out at this resolution. The galaxy is estimated to be of intermediate mass, with a moderate rate of star formation. The spectral properties suggest it is at an intermediate redshift.
