The galaxy presents as a disk galaxy, oriented approximately face-on to our line of sight. Prominent spiral arms are visible, exhibiting a relatively tightly wound structure. The color gradient suggests that the central bulge is more yellow-white, and there's a bluer hue in the spiral arms.

The galaxy does not exhibit an overly dominant bulge. The arms display some patchiness, likely indicating regions of active star formation. No clear signs of major mergers are visible, although the overall morphology shows a mild disturbance. The dust lanes are somewhat faint, adding to the complexity of the spiral structure.
