The galaxy appears to be a spiral galaxy, although the spiral arms are somewhat flocculent. A prominent central bulge is visible, contributing significantly to the overall luminosity. The winding of the spiral arms seems relatively tight. The galaxy is not viewed edge-on; instead, it is observed at an angle. It displays evidence of ongoing star formation, indicated by the blueish hue present in the spiral arms. There is no clear indication of a strong bar structure bisecting the central bulge. The galaxy appears relatively undisturbed, with no obvious signs of a major merger event, although the overall appearance suggests the possibility of minor gravitational interactions.
