The formulas for ##\nabla\times## in polar coordinates make calculations with radial vectors easy because all the hard work has been done in deriving the formulas. If you have not been given those formulas, and hence are required to derive them if you use them, there is no point in using them because the work involved in deriving them is greater than the work involved in just doing the whole calc in Cartesian coordinates.
Given that, the simplest way is just to do the calc in Cartesian coordinates. Since the usual coordinate names in Cartesian are ##x,y,z## I suggest you instead call your point ##\vec r##. Then the coordinates of ##\vec F(\vec r)## are ##(f(r)x,f(r)y,f(r)z)##, writing ##r## for ##\|\vec r\|##.
Then use the Cartesian formula for ##\nabla\times##:
$$\nabla\times\vec u=(\partial_x,\partial_y,\partial_z)\times (u_x,u_y,u_z)=(\partial_y u_z-\partial_zu_y)\hat i
+(\partial_z u_x-\partial_xu_z)\hat j
+(\partial_x u_y-\partial_yu_x)\hat k$$
where ##\partial_x## denotes ##\frac{\partial}{\partial x}## and ##u_x## is the ##x## coordinate of ##\vec u##.
The calc is quite short.