The observed galaxy presents as a disk-shaped structure with a noticeable central bulge. The bulge exhibits a yellowish-white hue, suggesting a population of older, cooler stars. A disk component is visible, displaying a bluer tint, potentially indicative of ongoing or recent star formation. There appears to be no strong indication of a spiral structure within the disk, but the resolution may limit the ability to resolve fine details. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or significant tidal interactions, it also does not seem to be forming stars at a very high rate. The galaxy is observed at a moderate redshift, placing it at a considerable cosmological distance. Its estimated mass is approximately 10^10 solar masses.
