The galaxy presents as a spiral, displaying a defined disk structure. Two distinct spiral arms emanate from the central bulge. The arms are tightly wound near the core but appear more diffuse toward the outer edges of the galactic disk. The galaxy exhibits a moderate bulge. There appears to be a weak bar structure visible in the central region. Coloration suggests on-going star formation within the spiral arms. Overall, the galaxy appears relatively isolated, with no obvious signs of recent or on-going major merger activity, although there are some minor disturbances in the disk.
