The galaxy appears as a moderately luminous, flattened spheroid. Its color profile exhibits a central concentration of light with a yellowish-orange hue, gradually fading towards the outer edges. There is some indication of a disk-like structure, but the system is overall smooth and elliptical in nature. The general morphology appears undisturbed, with no obvious signs of major mergers or tidal disruptions. Based on the redshift, the galaxy is at a significant cosmological distance, meaning we are seeing it as it was in the past. The central bulge seems to be composed of older stellar populations, while there might be some star formation activity occurring within a thin disk. However, the overall star formation rate is low, and the galaxy is likely dominated by passively evolving stars.
