The galaxy appears to be a spiral galaxy, presenting with a disk-like structure. Multiple spiral arms emanate from the galactic center. The arms are moderately wound, exhibiting a mix of medium and loose pitch angles. A central bulge is present, although not particularly prominent compared to the overall disk.

The galaxy appears to have a bar structure spanning its central region. The bar appears moderately pronounced. The overall color suggests a relatively young stellar population, with areas of active star formation visible within the spiral arms. There appears to be some minor asymmetry. This may suggest that some disturbance has occurred, although the galaxy is primarily intact.
