The galaxy exhibits a spiral structure, with prominent arms that are somewhat tightly wound. These arms are discernable and possess a clumpy morphology indicative of active star formation regions. There is a central bulge, but is not particularly prominent compared to the disk. The galaxy is viewed close to face-on, with very little tilt, giving a good view of its overall structure. There is a hint of bluer color within the spiral arms, suggestive of younger stellar populations. The overall appearance suggest a fairly well-defined spiral structure with ongoing star formation.
