This galaxy appears to be a spiral galaxy, observed at an angle that is tilted relative to our line of sight. The structure reveals a dominant disk component exhibiting distinct spiral arms. These arms present a tightly wound morphology. The central bulge is present, with a moderate size. The arms are populated with areas of active star formation as indicated by the bluish color. The image hints at a two-armed spiral structure. There is no evidence of a strong central bar. The overall structure suggests a relatively undisturbed morphology with no significant signs of a major merger, but it is likely experiencing minor gravitational disturbance.
