  We present an extensive catalog of non-parametric structural properties
derived from optical and mid-infrared imaging for 4585 galaxies from the MaNGA
survey. DESI and WISE imaging are used to extract surface brightness profiles
in the g, r, z, W1, W2 photometric bands. Our optical photometry takes
advantage of the automated algorithm AutoProf and probes surface brightnesses
that typically reach below 29 mag/arcsec^2 in the r band, while our WISE
photometry achieves 28 mag/arcsec^2 in the W1 band. Neighbour density measures
and central/satellite classifications are also provided for a large sub-sample
of the MaNGA galaxies. Highlights of our analysis of galaxy light profiles
include: (i) an extensive comparison of galaxian structural properties that
illustrates the robustness of non-parametric extraction of light profiles over
parametric methods; (ii) the ubiquity of bimodal structural properties
suggesting the existence of galaxy families in multiple dimensions; and, (iii)
an appreciation that structural properties measured relative to total light,
regardless of the fractional level, are uncertain. We study galaxy scaling
relations based on photometric parameters, and present detailed comparisons
with literature and theory. Salient features of this analysis include the
near-constancy of the slope and scatter of the size-luminosity and size-stellar
mass relations for late-type galaxies with wavelength, and the saturation of
the central surface density, measured within 1 kpc, for elliptical galaxies
with M* > 10.7 Msol (corresponding to Sigma_1 ~ 10^{10} Msol/kpc^2). The
multi-band photometry, environmental parameters, and structural scaling
relations presented are useful constraints for stellar population and galaxy
formation models.
