The galaxy presents as a relatively compact and bright object. It exhibits a largely smooth morphology, suggesting an elliptical or lenticular type. There is a slight elongation observed, though it appears generally rounded. No distinct spiral arms or significant dust lanes are discernible at this resolution. The color profile indicates an older stellar population, with light concentrated in the redder wavelengths. Based on its red shift, this is a galaxy in the distant universe. There is no apparent sign of a major ongoing merger event, though the morphology suggests some sort of past interaction or minor disturbance.