In this work, we propose a prototype for a scalable software infrastructure to enable the retrieval and analysis of galaxy images from public astronomical archives. We implement and deploy our prototype to estimate the position angles of $6 \times 10^{6}$ galaxies in multiple optical to near-infrared wavelengths. The position angle determination is performed using Radon transforms, and thus it is obtained in a fully non-parametric way, reducing possible model-dependent biases. Finally, these measurements can be adopted to further reveal dark matter signatures and constrain important cosmological parameters of the models we use to explain our Universe.