The galaxy presents as a relatively face-on spiral galaxy, observed at a redshift that places it at a considerable distance. The morphology suggests a flattened disk structure. There is a bright central bulge that appears smooth and elliptical in shape, with a color gradient transitioning from yellow/orange at the core to a bluer hue in the outer regions of the disk. A dark dust lane that is obscuring the central bulge suggests that it is a spiral galaxy viewed at an angle. A faint galactic halo extends beyond the visible disk, suggesting a surrounding population of older stars or diffuse gas. The spiral arms appear somewhat tightly wound, indicating it could be an Sa or Sb type galaxy. The blue color in the outer regions suggests ongoing star formation within the spiral arms. There is no evidence of any major disturbances or mergers.
