This galaxy appears to be a relatively smooth, elliptical system. It exhibits a bright, concentrated core region that fades gradually outward, suggesting a high degree of stellar population density in the center. The galaxy's overall shape is quite round, showing minimal deviation from a perfect sphere. There is no discernible disk structure or prominent spiral arms. No indications of major mergers or significant tidal disturbances in its morphology are seen. The galaxy displays a moderate amount of blue color in its halo, possibly indicating ongoing but limited star formation activity. The overall redshift suggests that this is an object at significant cosmological distance.
