This galaxy appears to be an elliptical galaxy at a redshift of approximately 0.22, based on photometric redshift estimations. The galaxy is dominated by older stellar populations, exhibiting a smooth, round morphology. The light is concentrated towards the center, indicating a high degree of central mass concentration. There is no visible disk structure or spiral arms. The galaxy appears to have a very low star formation rate based on its red color. There is no apparent interaction or merger activity. The galaxy is not perfectly round; there is a very slight elongation.
