The galaxy presents as a spiral type, inclined at an angle such that a portion of the disk structure is apparent. Two primary spiral arms are visible, exhibiting a medium to loose winding pattern. A bar structure is subtly present across the central bulge of the galaxy. The bulge itself appears moderate in size, exhibiting a yellowish color, suggesting an older stellar population. The spiral arms are characterized by a bluer hue, indicative of ongoing star formation. There is no apparent major merger occurring, although signs of minor disturbances are visible on the outskirts of the disk. The overall structure suggests a galaxy undergoing active, but not extremely high, star formation.
