The galaxy exhibits a disk-like structure, viewed at an intermediate inclination angle. There is a noticeable central bulge. Faint spiral arm structures are visible within the disk, appearing somewhat tightly wound. Star formation regions are present and appear clumpy, showing a blue-green hue concentrated within the spiral arms. Dust lanes are also visible within the disk. The outer regions of the galaxy's disk fade gradually, indicating a less dense distribution of stars and gas at larger radii. The galaxy appears undisturbed, with no obvious signs of a major merger or tidal interactions.
