The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution exhibits a nearly circular morphology, appearing quite rounded in shape. There's a gradual decrease in luminosity from the core outwards, suggesting a lack of distinct spiral arms or prominent features typically associated with disk galaxies. The color profile indicates a redder hue in the central region, transitioning to slightly bluer tones towards the outer edges. There is no indication of any major ongoing merger events or significant tidal disturbances. The galaxy seems to be a spheroid, as expected from a high redshift galaxy.
