  We proceed to derive equations for the symmetric tensor of the second rank on
the basis of the Bargmann-Wigner formalism in a straightforward way. The
symmetric multispinor of the fourth rank is used. It is constructed out of the
Dirac 4-spinors. Due to serious problems with the interpretation of the results
obtained on using the standard procedure we generalize it and obtain the spin-2
relativistic equations, which are consistent with the previous one. The
importance of the 4-vector field (and its gauge part) is pointed out.
