The galaxy exhibits a clear spiral structure, although the spiral arms appear somewhat flocculent and not as tightly wound. There is evidence of a bar feature spanning a significant portion of the galaxy's central region. The bulge component appears relatively small to moderate in size compared to the overall disk. The galaxy disk is tilted relative to our line of sight. There are no obvious signs of major recent merger activity; however, a slight asymmetry or minor disturbance in the outer regions might suggest a past interaction. Star formation activity appears to be ongoing. The core of the galaxy is bright with a yellow hue, and this fades out as you move to the outer arms.
