The galaxy exhibits a spiral morphology, appearing nearly face-on. Multiple spiral arms emanate from a central bulge. The arms are tightly wound and possess a grainy texture suggesting regions of star formation. The central bulge appears bright and concentrated, diminishing in intensity towards the outer disk. A bar structure is faintly visible traversing the central region. The overall color of the galaxy appears bluish, possibly indicating a population of younger stars. A slight asymmetry is visible in the outer regions of the disk, possibly indicating a minor gravitational interaction with a smaller galaxy, or some disturbance to the structure.
