The galaxy presents as a moderately luminous, elliptical object with a significant redshift, indicating substantial distance. It exhibits a generally smooth morphology with a central bulge that appears elongated along one axis. The color gradient suggests a population of older stars, particularly concentrated in the central region which appears more yellow. There is little evidence of spiral arms or active star formation regions in the visible light. There is a hint of a slight disturbance in the overall structure, but its overall morphology is generally undisturbed. Based on its apparent magnitude, the galaxy likely has a stellar mass around 10^10 solar masses.
