  We present an analysis of the chiral property of 1,621 field galaxies having
radial velocity 3,000 km/s to 5,000 km/s . A correlation between the chiral
symmetry breaking and the preferred alignment of galaxies in the leading and
trailing structural modes is studied using chi-square, auto-correlation and the
Fourier tests. We noticed a good agreement between the random alignment of the
position angle (PA) distribution and the existence of chirality in both the
leading and trailing arm galaxies. Chirality is found stronger for the
late-type spirals (Sc, Scd, Sd and Sm) than that of the early-types (Sa, Sab,
Sb and Sbc). A significant dominance (17% $\pm$ 8.5%) of trailing modes is
noticed in the barred spirals. In addition, chirality of field galaxies is
found to remain invariant under the global expansion. The PA-distribution of
the total trailing arm galaxies is found to be random, whereas preferred
alignment is noticed for the total leading arm galaxies. It is found that the
rotation axes of leading arm galaxies tend to be oriented perpendicular the
equatorial plane. A random alignment is noticed in the PA-distribution of
leading and trailing spirals.
