The galaxy presents as a spiral structure with a notable disk. The arms are well-defined, displaying a prominent two-armed pattern. The winding of the spiral arms appears to be of medium tightness, neither tightly wound nor loosely sprawling. There is evidence of a bar feature spanning across the center of the galaxy; although it is not exceptionally strong, its presence is clear. The galaxy exhibits a moderate bulge size, neither dominating the disk nor being insignificant. There are no obvious signs of major merging activity, but a hint of minor disturbance cannot be completely ruled out.
