The galaxy presents as a spiral type, although the disk appears somewhat disturbed. The spiral arms are clearly present, with a high degree of certainty. There is a faint blueish tinge to the arms. A central bulge is visible but not dominant. There is no indication of a strong bar structure. The overall impression suggests a disk galaxy with ongoing, albeit not extreme, star formation. There is some evidence of interactions, perhaps a minor disturbance, but no clear signs of a major ongoing merger.
