The galaxy exhibits a distinct spiral structure. The arms are tightly wound and span a considerable extent. Two prominent spiral arms are visible, emanating from a central bulge. The bulge appears moderate in size compared to the overall galactic disk. The disk is not edge-on. Star formation appears active within the spiral arms, implied by the bluish hue. No significant bar structure is clearly observed. The galaxy is mostly undisturbed with a slight possibility of minor disturbance, as there appear to be no large tidal tails or strong asymmetries. The galaxy’s overall appearance suggests a mature, well-formed spiral galaxy undergoing ongoing star formation.
