Venus is similar to the Earth in size， mass， composition and distance to the sun. However， Venus has neither plate tectonics nor dynamo that exists on the Earth. The lithosphere of Venus is very thick based on its topography and gravity. The admittance and correlation between Venusian geoid and topography are very high， suggesting that they are strongly influenced by the internal dynamical process of Venus. Analyses show that there may be 10 Hawaii-like mantle plumes in Venusian mantle. Data from Venus Express has shown evidence for recent active volcanism among several of these plumes. The distribution of impact craters on Venus shows that Venusian surface has a young age and the age is averaged about 500 Ma， suggesting that Venus may have experienced a global resurfacing event. However， whether this resurfacing is catastrophic or equilibrium is still under debate. It is also unclear whether Venus had plate tectonics in the past， is it always in stagnant lid regime， or might it have an entirely different mode？In general， the style of mantle convection on Venus is quite different from that of the Earth which is manifested by the plate tectonics. Here we reviewed the main observations including gravity， topography and surface tectonics which provide constrains on the interior structure and dynamics of Venus， and recent advance in the interior structure and dynamics of Venus. This review aims to provide new insights into the interior dynamics of Venus.