The galaxy presents as a spiral galaxy with a moderately sized central bulge. The spiral arms appear distinct and exhibit a two-armed structure. The winding of the spiral arms is neither tightly wound nor loosely structured, but instead appears to exhibit moderate winding. A bar structure is present across the center of the bulge, classified as a moderately strong bar. The galactic disk displays a significant inclination relative to our line of sight. The galaxy shows no strong indication of major ongoing merger activity but there are some minor signs of disturbances.
