No. While initial rotation of Venus during primordial times was probably fast and prograde, Venus has been in its present configuration of slow retrograde motion within the age of the Solar System, possibly during the first billion years (Correia, 2003; bit.ly/spinofvenus). It is believed that the present motion of Venus is a steady state between gravitational tides and thermally driven atmospheric tides, as well as tidal dissipation effects due to proximity to the Sun (Correia, 2010; bit.ly/tidalevol).