The galaxy presents as a luminous, elliptical structure. The core is a bright, concentrated yellow-orange hue, suggesting a significant population of older stars. There is a gradual decrease in luminosity moving outward from the core. It appears somewhat elongated, with the major axis approximately twice as long as the minor axis. There are no clearly defined spiral arms or prominent dust lanes visible in this image, suggesting a relatively smooth distribution of stellar mass. Faint, diffuse extensions appear at the extremities of the major axis. Overall, the galaxy's morphology indicates it is likely an elliptical galaxy with a relatively old stellar population and a significant mass. There are no obvious signs of recent major mergers or significant star formation activity, though subtle minor disturbances cannot be ruled out based on this image alone. The redshift indicates that the galaxy is distant.
