The galaxy presents a moderately inclined disk, exhibiting a spiral structure. The spiral arms appear somewhat tightly wound, suggesting an Sa or Sb type morphology. A substantial central bulge is evident, contributing significantly to the galaxy's overall luminosity. The disk shows evidence of active star formation, indicated by the blue hue throughout the disk. There are some indications of minor disturbances in the structure, which could be from a tidal interaction or minor merger. A strong bar structure is not evident, and the arms appear two-armed but not perfectly symmetric.
