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Context: The Supernova Remnants (SNRs) known in the Large Magellanic Cloud(LMC) show a variety of morphological structures in the different wavelengthbands. This variety is the product of the conditions in the surrounding mediumwith which the remnant interacts and the inherent circumstances of thesupernova event itself.  Aims: This paper performs a multi-frequency study of the LMC SNR J0530-7007by combining Australia Telescope Compact Array (ATCA), Molonglo ObservatorySynthesis Telescope (MOST), R\"ontgensatellit (ROSAT) and Magellanic CloudsEmission Line Survey (MCELS) observations.  Methods: We analysed radio-continuum, X-ray and optical data and present amulti-wavelength morphological study of LMC SNR J0530-7007. Results We findthat this object has a shell-type morphology with a size of 215"x180" (52 pc x44 pc); a radio spectral index (alpha=-0.85+-0.13); with [Sii]/Halpha > 0.4 inthe optical; and the presence of non-thermal radio and X-ray emission.  Conclusions: We confirmed this object as a bona-fide shell-type SNR which isprobably a result of a Type Ia supernova.

Multi-Frequency Study of Supernova Remnants in the Large Magellanic Cloud. The case of LMC SNR J0530-7007