The galaxy presents a distinct spiral morphology. It exhibits tightly wound spiral arms emanating from a central bulge region. The arms are not uniformly distributed but show a clumpy structure, suggesting regions of active star formation. The central bulge appears relatively small and bright. There is some evidence of a bar-like structure bisecting the bulge. The overall color of the galaxy indicates the presence of both younger, bluer stellar populations within the arms and older, redder populations concentrated towards the central bulge. The disk is oriented at a slight angle relative to our line of sight. The image suggests a galaxy that is relatively isolated, without any signs of major interactions or mergers. There may be some minor disturbances or asymmetries in the outer arms. The image exhibits several distinct arms, which, while tightly wound, appear to branch and segment across the galaxy disk.
