The galaxy presents as a disk galaxy, likely observed at a moderate inclination. The central bulge is discernible, appearing relatively small to moderate in size. Faint spiral arm structures are visible, hinting at ongoing star formation. The blue hues observed within the disk suggest the presence of young, hot stars. There are no obvious signs of any major mergers; however, some disturbances appear. Overall, the galaxy shows a mix of smooth and more structured regions, suggesting both older stellar populations and more recent star formation. The galaxy does not present as barred.
