The galaxy presents as a moderately luminous, ellipsoidal structure with a redshift suggesting significant distance. Morphologically, it appears smooth and relatively rounded, with a dominant central bulge exhibiting a yellowish hue, indicative of an older stellar population. There is evidence of a secondary concentration of light, which could suggest a minor interaction or merger event. The overall color indices suggest a population of intermediate to old stars with relatively low ongoing star formation. There is some irregularity in the surrounding galactic halo, potentially from past or ongoing accretion. The faint outer regions suggest a gradual decrease in stellar density away from the core, typical of elliptical galaxies at this redshift.
