The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or lenticular galaxy at an intermediate redshift. The light distribution is dominated by a bright, yellowish-orange core that gradually fades into a less luminous, bluish-white halo. There are no discernible spiral arms or dust lanes visible. The overall shape appears close to circular, with a slight suggestion of elongation. There is no evidence of a major merger event, though minor disturbances cannot be ruled out. Color gradients suggest older stellar populations are concentrated in the center, with slightly younger stars in the outer regions.
