The galaxy exhibits a distinct disk-like structure. Spiral arms are present, displaying a somewhat flocculent pattern with hints of blue star formation regions. The central bulge appears moderate in size and exhibits a smoother texture than the arms. A bar-like feature is prominent along the galaxy's central region, but is not very pronounced. There is no indication of major interactions or a significant merger event from the galaxy’s morphology. The overall structure suggests a well-defined but modestly disturbed spiral morphology. The galaxy is not seen edge-on and has a relatively large angular size, which could indicate that it is reasonably close by.
