  We search for Milky Way-like galaxies among a sample of approximately 500
galaxies. The characteristics we considered of the candidate galaxies are the
following: stellar mass M_star, optical radius R_25, rotation velocity V_rot,
central oxygen abundance (O/H)_0, and abundance at the optical radius
(O/H)_R25. If the values of R_25 and M_star of the galaxy were close to that of
the Milky Way, then the galaxy was referred to as a structural Milky Way
analogue (sMWA). The oxygen abundance at a given radius of a galaxy is defined
by the evolution of that region, and we then assumed that the similarity of
(O/H)_0 and (O/H)_R25 in two galaxies suggests a similarity in their evolution.
If the values of (O/H)_0 and (O/H)_R25 in the galaxy were close to that of the
Milky Way, then the galaxy was referred to as an evolutionary Milky Way
analogue (eMWA). If the galaxy was simultaneously an eMWA and sMWA, then the
galaxy was considered a Milky Way twin. We find that the position of the Milky
Way on the (O/H)_0 - (O/H)_R25 diagram shows a large deviation from the general
trend in the sense that the (O/H)_R25 in the Milky Way is appreciably lower
than in other galaxies of similar (O/H)_0. This feature of the Milky Way
evidences that its (chemical) evolution is not typical. We identify four
galaxies (NGC~3521, NGC~4651, NGC~2903, and MaNGA galaxy M-8341-09101) that are
simultaneously sMWA and eMWA and can therefore be considered as Milky Way
twins. In previous studies, Milky Way-like galaxies were selected using
structural and morphological characteristics, that is, sMWAs were selected. We
find that the abundances at the centre and at the optical radius (evolutionary
characteristics) provide a stricter criterion for selecting real Milky Way
twins
