  The DESI Legacy Survey is a digital sky survey with a large footprint
compared to other Earth-based surveys, covering both the Northern and Southern
hemispheres. This paper shows the distribution of the spin directions of spiral
galaxies imaged by DESI Legacy Survey. A simple analysis of dividing nearly
1.3$\cdot10^6$ spiral galaxies into two hemispheres shows a higher number of
galaxies spinning counterclockwise in the Northern hemisphere, and a higher
number of galaxies spinning clockwise in the Southern hemisphere. That
distribution is consistent with previous observations, but uses a far larger
number of galaxies and a larger footprint. The larger footprint allows a
comprehensive analysis without the need to fit the distribution into an a
priori model, making this study different from all previous analyses of this
kind. Fitting the spin directions of the galaxies to cosine dependence shows a
dipole axis alignment with probability of $P<10^{-5}$. The analysis is done
with a trivial selection of the galaxies, as well as simple explainable
annotation algorithm that does not make use of any form of machine learning,
deep learning, or pattern recognition. While further work will be required,
these results are aligned with previous studies suggesting the possibility of a
large-scale alignment of galaxy angular momentum.
