The galaxy appears as a singular, roughly circular object in the image. Its color profile leans toward the green end of the spectrum, suggesting a mix of stellar populations. The smooth, concentrated light distribution indicates a lack of significant spiral arm structure or other major morphological features. There might be a very slight asymmetry to the light distribution, with a hint of elongation. However, the smoothness appears to dominate. The lack of obvious tidal tails or strong disturbances suggests that this galaxy is not currently undergoing a major merger, though a minor interaction cannot be ruled out. Considering the estimated redshift, this galaxy is a significant distance away, making detailed morphological assessment challenging. The overall impression is that of a relatively quiescent, elliptical or lenticular galaxy.
