  HD~105 is a nearby, pre-main sequence G0 star hosting a moderately bright
debris disc ($L_{\rm dust}/L_{\star} \sim 2.6\times10^{-4}$). HD~105 and its
surroundings might therefore be considered an analogue of the young Solar
System. We refine the stellar parameters based on an improved Gaia parallax
distance, identify it as a pre-main sequence star {with an age of
50~$\pm$~16~Myr}. The circumstellar disc was marginally resolved by
\textit{Herschel}/PACS imaging at far-infrared wavelengths. Here we present an
archival ALMA observation at 1.3~mm, revealing the extent and orientation of
the disc. We also present \textit{HST}/NICMOS and VLT/SPHERE near-infrared
images, where we recover the disc in scattered light at the $\geq$~5-$\sigma$
level. This was achieved by employing a novel annular averaging technique, and
is the first time this has been achieved for a disc in scattered light.
Simultaneous modelling of the available photometry, disc architecture, and
detection in scattered light allow better determination of the disc's
architecture, and dust grain minimum size, composition, and albedo. We measure
the dust albedo to lie between 0.19 and 0.06, the lower value being consistent
with Edgeworth-Kuiper belt objects.
