The galaxy presents as a centrally concentrated light source with a notable degree of smoothness in its overall appearance. The central region exhibits a brighter, more intense emission, suggesting a higher density of stars or ionized gas. The overall shape appears elliptical, with a deviation from perfect circularity. There is a slight elongation visible. No distinct spiral arms or other features are readily apparent in this observation. There is a minor indication of possible disturbance in the halo of the galaxy. The color profile indicates stronger emission in the green wavelengths. This is likely due to the composition of the galaxy and the redshift. It is potentially an elliptical galaxy at an extreme redshift.
