The galaxy presents as a spiral type with well-defined spiral arms emanating from a central bulge. The arms appear relatively loose, and tracing them suggests primarily a two-armed structure. There's a slight asymmetry in the arm structure and brightness distribution, possibly indicating a minor gravitational interaction or disturbance. The central bulge is not overly prominent, exhibiting a moderate size relative to the overall galactic disk. A bar structure appears to extend through the center, but it is not very strong. In the arms, pockets of star forming activity are occurring as can be seen by the bluish color of the star clusters in the spiral arms.