Without further information I would guess that you are talking about the Euler integration scheme which is a method for a numerical approximation of an ordinary differential equation.
If you are further talking about Newtonian mechanics, you mean that there is a point mass of mass $m$ whose behaviour is described by the equation $$ F = m * a $$ Force = mass times accelaration. This is an ordinary differential equation of second order for the position of the point mass as a function of time $t$, $S(t)$, because we have $$ S''(t) = a(t) $$ that is the first derivative of $S$ is the velocity $v(t)$, and the second is the acceleration $a(t)$. In order to get a unique solution, we need to specify initial conditions for both $S(t)$, $$ S(t =0) = S_0 $$ which is the initial position and for $v(t)$, $$ v(t = 0) = v_0 $$ which is the initial velocity of the point mass. Now you can prescribe the force $F(t)$ as a differentiable function of time and calculate the position $S(t)$ numerically using the Euler method. If you set the force to zero, then you have zero acceleration and the unique solution in closed form is $$ S(t) = S_0 + v_0 t $$ In this case the numerical approximation via the Euler method will coincide with the solution obtained in closed form. But in general there will be an approximation error.
HTH