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We present an extensive catalog of non-parametric structural propertiesderived from optical and mid-infrared imaging for 4585 galaxies from the MaNGAsurvey. DESI and WISE imaging are used to extract surface brightness profilesin the g, r, z, W1, W2 photometric bands. Our optical photometry takesadvantage of the automated algorithm AutoProf and probes surface brightnessesthat typically reach below 29 mag/arcsec^2 in the r band, while our WISEphotometry achieves 28 mag/arcsec^2 in the W1 band. Neighbour density measuresand central/satellite classifications are also provided for a large sub-sampleof the MaNGA galaxies. Highlights of our analysis of galaxy light profilesinclude: (i) an extensive comparison of galaxian structural properties thatillustrates the robustness of non-parametric extraction of light profiles overparametric methods; (ii) the ubiquity of bimodal structural propertiessuggesting 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 scalingrelations based on photometric parameters, and present detailed comparisonswith literature and theory. Salient features of this analysis include thenear-constancy of the slope and scatter of the size-luminosity and size-stellarmass relations for late-type galaxies with wavelength, and the saturation ofthe central surface density, measured within 1 kpc, for elliptical galaxieswith M* > 10.7 Msol (corresponding to Sigma_1 ~ 10^{10} Msol/kpc^2). Themulti-band photometry, environmental parameters, and structural scalingrelations presented are useful constraints for stellar population and galaxyformation models.

MaNGA galaxy properties -- I. An extensive optical, mid-infrared photometric, and environmental catalogue