The galaxy presents as a spiral structure, inclined at an angle. Spiral arms appear present. While not fully edge-on, the disk morphology is visible. A distinct central bulge is observed, exhibiting a moderate size relative to the disk. The spiral arms themselves appear somewhat tightly wound. Two predominant arms are identifiable. The morphology indicates the presence of a barred structure across the galactic center. Some indications of disturbance or interaction are present in the disk, although no clear merging events are visible. The galaxy displays a blue hue indicative of on-going star formation activity.
