The galaxy presents a generally smooth, elliptical morphology. The light distribution appears concentrated towards the center, with a gradual decrease in intensity outward. The object exhibits a dominant yellow-orange color, suggesting an older stellar population with relatively little ongoing star formation. There is no discernible disk structure or spiral arms, and no obvious signs of a recent major merger, although a minor disturbance cannot be ruled out. The shape is predominantly round. The relatively high red shift indicates that this galaxy is a distant object.