The galaxy presents as a centrally concentrated, relatively smooth object. It exhibits a spheroidal morphology with a high degree of radial symmetry. A slight elongation is observed, deviating marginally from a perfectly circular profile. Color gradients are subtle, showing a bluer core that fades to redder hues in the outer regions. No distinct spiral arms or prominent dust lanes are visible. The galaxy appears relatively isolated, showing no obvious signs of major interaction or ongoing merging activity, though some minor disturbances cannot be ruled out. Its overall appearance is consistent with that of an elliptical galaxy at a redshift that places it at a considerable distance. The effective radius is around 1.5 kiloparsecs. The mass is probably around 10^8 solar masses. Star formation is expected to be quite low.
