The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and featureless morphology. It presents a near-perfect rounded shape, suggesting a minimal degree of rotational support. The color profile indicates a strong central concentration of older stellar populations. The redshift implies a considerable distance. There is little to no visible evidence of ongoing star formation within the galaxy itself. The lack of prominent spiral arms or dust lanes further reinforces the classification of this galaxy as an elliptical. There is no evidence that this galaxy is currently undergoing a merger, although minor disturbances cannot be ruled out at this resolution.
