The galaxy presents a face-on spiral morphology. Two prominent spiral arms are distinctly visible, exhibiting a medium winding pattern. A central bar structure is observed bisecting the nucleus, which appears bright and somewhat diffused. The arms themselves show clumpy structures, suggesting active star formation regions. Overall, the galaxy's disk appears slightly disturbed, perhaps exhibiting signs of minor interaction or internal activity. The bulge is moderate in size and blends smoothly with the disk, rather than being distinctly set apart. The colour profile indicates a relatively high level of star formation. 
