The galaxy presents as a relatively face-on spiral with a prominent central bulge exhibiting a yellow-orange hue, suggestive of an older stellar population. Surrounding the bulge, there is a disk component with a mottled appearance, indicative of spiral arm structures. The arms themselves are not sharply defined but discernible through variations in color and brightness. Hints of bluer regions are present within the spiral arms, implying ongoing star formation activity. The overall morphology appears relatively undisturbed, with no obvious signs of a recent major merger, although subtle asymmetries could indicate minor interactions.
