The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light profile. The light is slightly elongated. There is a color gradient from the core to the outer regions. The core exhibits a bluer hue, suggesting the presence of younger stellar populations or ongoing star formation, while the outer regions appear redder, indicative of older, cooler stars. There is no discernable spiral arm structure, bar or dust lane. The galaxy appears relatively undisturbed, without evidence of any major merger events, strong tidal features or any ongoing starburst activity. The redshift suggests this galaxy is at a considerable distance, however the absolute magnitudes suggest it is a relatively luminous galaxy.
