This galaxy appears to be a spiral galaxy, observed at an angle somewhat between face-on and edge-on. The disk is clearly visible, displaying prominent spiral arm structures. These arms exhibit a tightly wound morphology. There is no evidence of a strong central bar. The galaxy possesses a noticeable bulge, which is classified as moderately sized compared to the overall galaxy. The presence of spiral arms and the disk-like appearance suggest active star formation is occurring within the galaxy, concentrated along the spiral arms. There may be some interactions with other objects.
