The galaxy presents a disk-like morphology, viewed at an oblique angle. The dominant feature appears to be ongoing star formation, evidenced by numerous bright, blue-tinged star-forming regions scattered throughout the disk. The central bulge appears to be relatively small, and its contribution to the overall luminosity is subordinate to that of the disk. There's a possible indication of disrupted morphology, but it's very slight and the system looks mostly undisturbed. It appears that the outer parts of the disk are more active with star formation than the inner parts. There is a subtle bar-like feature that might cut across the galaxy's center. Spiral arm structures are present within the disk and are fairly prominent. The spiral structure is somewhat flocculent, rather than grand design.
