The galaxy presents a largely smooth and rounded morphology. The light distribution appears relatively uniform, lacking prominent spiral arms or a distinct central bulge. There is a suggestion of a slight elongation, but it's largely spheroid. Its color profile leans toward the red end of the spectrum, indicating a potentially older stellar population and a lower rate of current star formation. No evidence of a major merger or significant tidal disturbances is apparent in the image. Based on its apparent size and redshift, it is likely a relatively massive galaxy. 
