This galaxy appears to be a relatively smooth, elliptical galaxy. Its light profile suggests a centrally concentrated stellar population with a gradual decrease in luminosity towards the outer regions. There is no evidence of distinct spiral arms or a prominent disk structure. The galaxy exhibits a slightly elongated shape, appearing more rounded than cigar-shaped, and shows no obvious signs of major mergers or significant tidal disturbances. Its color index indicates it is a red galaxy, which is typical for elliptical galaxies, and has a large mass estimate. This suggests that star formation is relatively suppressed compared to the past. The high red-shift value indicates it is relatively far away.