The galaxy presents as a spiral type, likely a grand design spiral exhibiting two prominent and well-defined arms. The winding of these spiral arms appears moderately tight. A central bulge is visible, and it appears moderate in size relative to the galactic disk. There is no obvious presence of a strong bar structure, although a weak bar cannot be ruled out. There is a slight possibility of a minor disturbance due to a possible interaction with a nearby galaxy, although this might also be the artifact of merging from an earlier disturbance that is now subsiding.
