The galaxy presents as a generally smooth, centrally concentrated object. It exhibits an elliptical morphology with a moderate degree of roundness. The color gradient transitions from a yellowish-white core to a reddish-orange outer halo. No distinct spiral arm structures or prominent dust lanes are discernible. There are no signs of any major mergers or significant tidal disturbances, although the galaxy appears to be slightly asymmetric and may be experiencing minor gravitational interactions. Given the object's redshift, this galaxy is relatively distant. The galaxy has a estimated mass of over 100 billion times the mass of the sun, and a low star formation rate.
