The galaxy exhibits a spiral morphology with a prominent central bulge. The spiral arms appear loosely wound and extended, hinting at a relatively late-type classification. Evidence of star formation is suggested by the slightly blue hue within the arms. The disk is not perfectly face-on, displaying a degree of inclination to our line of sight. A bar-like structure bisects the bulge, possibly influencing the shape and dynamics of the spiral arms. The galaxy's structure is somewhat disrupted, indicating potential tidal interactions or a past merger event.
