The galaxy presents as a spiral type, characterized by the presence of distinct spiral arms. Two primary arms appear prominent, exhibiting a relatively medium winding pattern as they extend from the central region. The central bulge is discernible, possessing a moderate size compared to the overall galactic disk. Within the disk, there is evidence of ongoing star formation, indicated by variations in color and brightness along the spiral arms, suggestive of active regions. There is a potential for a weak bar-like structure in the center, although a more detailed inspection would be needed to make a final judgment. Additionally, the overall morphology of the galaxy does not show significant signs of recent major disturbance or merger activity, despite the presence of some unevenness in the arm structure, which could indicate minor interactions.
