The galaxy presents a flattened, disk-like structure oriented approximately edge-on relative to our line of sight. Prominent spiral arm features are evident, displaying a somewhat flocculent and patchy morphology. The spiral arms appear blue, suggesting the presence of recent or ongoing star formation activity within them. A bar structure bisects the central region of the galaxy, contributing to a somewhat distorted or asymmetrical appearance in the inner disk. A weak bulge component is observed, only slightly concentrated. Some subtle irregularities in the galaxy's outer regions indicate minor gravitational disturbance or interaction. The overall appearance suggests a relatively late-type spiral galaxy with actively forming stars and signs of dynamical interaction.
