There is a growing consensus that Venus is seismically active, although its level of seismicity could be very different from that of Earth due to the lack of plate tectonics. Here, we estimate upper and lower bounds on the expected annual seismicity of Venus by scaling the seismicity of the Earth. We consider different scaling factors for different tectonic settings and account for the lower seismogenic zone thickness of Venus. We find that 11 - 34 venusquakes >=Mw5 per year are expected for an inactive Venus, where the global seismicity rate is similar to that of continental intraplate seismicity on Earth. For the active Venus scenarios, we assume that the coronae, ridges, and rifts of Venus are currently seismically active. This results in 126 - 391 venusquakes >=Mw5 annually as a realistic lower bound and 465 - 1446 venusquakes >=Mw5 as a maximum upper bound for an active Venus.