  We present a detailed study of new Australia Telescope Compact Array (ATCA)
and XMM-Newton observations of LHA 120-N 70 (hereafter N 70), a spherically
shaped object in the Large Magellanic Cloud (LMC) classified as a superbubble
(SB). Both archival and new observations were used to produce high quality
radio-continuum, X-ray and optical images. The radio spectral index of N 70 is
estimated to be $\alpha=-0.12\pm 0.06$ indicating that while a supernova or
supernovae have occurred in the region at some time in the distant past, N70 is
not the remnant of a single specific supernova. N70 exhibits limited
polarisation with a maximum fractional polarisation of 9% in a small area of
the north west limb. We estimate the size of N 70 to have a diameter of 104 pc
($\pm 1$ pc). The morphology of N 70 in X-rays closely follows that in radio
and optical, with most X-ray emission confined within the bright shell seen at
longer wavelengths. Purely thermal models adequately fit the soft X-ray
spectrum which lacks harder emission (above 1 keV). We also examine the
pressure output of N 70 where the values for the hot (PX) and warm (PHii) phase
are consistent with other studied Hii regions. However, the dust-processed
radiation pressure (PIR) is significantly smaller than in any other object
studied in Lopez et al. (2013). N70 is a very complex region that is likely to
have had multiple factors contributing to both the origin and evolution of the
entire region.
