The galaxy appears as a disk-shaped structure, viewed at an oblique angle. The central region exhibits a bright, concentrated light, suggesting a prominent galactic nucleus. Surrounding this core, the disk shows a slightly clumpy structure. The overall color gradient transitions from a bluer hue in the central regions to a redder tone in the outer edges of the disk. There are signs of potential tidal disturbances or arm features. The overall structure indicates that the galaxy is likely an early spiral galaxy.