The galaxy presents as a face-on spiral, exhibiting a prominent central bulge. The bulge appears moderately sized, contributing significantly to the overall luminosity. The spiral arms are well-defined and numerous, with a tightly wound morphology. Star formation is evident within the arms, indicated by bluish hues. There is a slight asymmetry in the distribution of the spiral arms. The disk structure is clearly visible and not seen as edge-on. There is no clear evidence of any major merging events.
