The galaxy exhibits a prominent spiral structure. Two spiral arms are clearly discernible, tracing outward from a central bulge. The arms appear relatively open, exhibiting a moderate pitch angle. The central bulge is significant, and its color suggests a substantial population of older stars. It is difficult to resolve the exact shape of the bulge. The color of the spiral arms suggests ongoing star formation, indicated by bluer regions. The galaxy displays no obvious signs of major interaction or significant morphological disturbance, although there are a few regions of brighter intensity in the spiral arms. No obvious bar structure is visible in the image. The overall appearance suggests an intermediate-mass spiral galaxy at a moderate distance.
