The galaxy presents as a spiral with tightly wound arms. The spiral arms have a flocculent appearance, exhibiting a patchy structure with varying degrees of stellar density and color. The central bulge appears prominent, exhibiting a smooth and concentrated light profile, suggesting an older stellar population. There is a slight elongation and asymmetry to the galactic disk. The color gradient transitions from a yellow-white core to bluer spiral arms. The bluer arms suggest the presence of ongoing star formation.
