The galaxy presents an elliptical morphology, appearing largely smooth and featureless. It displays a moderate concentration of light towards the center. The color gradient transitions from a bluer hue at one end to a yellower hue at the other. The relative smoothness suggests that it is composed of an older stellar population. Given its red shift and the inferred star formation rate, it is likely a relatively massive galaxy with subdued star formation activity. The galaxy exhibits a somewhat elongated shape. There is no obvious evidence of spiral arms or a disk structure. Any potential distortions are minor, suggesting that it has not undergone a major merger in recent history.
