  We present an analysis of physical and morphological properties of an
interacting pair of dwarf galaxies UGC 4703 located at the vicinity of an
isolated Milky-Way (MW) type spiral galaxy NGC 2718. Based on the comparison of
physical and morphological properties with that of the Large and Small
Magellanic Clouds (LMC and SMC), we report that the UGC 4703 pair-NGC 2718
system is probably an LMC-SMC-MW analogue. Located at a sky projected distance
of 81 kpc from NGC 2718, we find that UGC 4703 is clearly interacting with its
nearby smaller mass companion UGC 4703B forming a bridge of stellar stream
between them. Total B-band luminosity of UGC 4703 and its companion is -17.75
and -16.25 mag, respectively. We obtained HI 21-cm line data of UGC 4703 using
the GMRT to get a more detailed view of neutral hydrogen (HI) emission. The HI
image revealed evidence of interaction between the dwarf galaxy pair but no
extended emission, like Magellanic Stream (MS), was detected between NGC 2781
and the UGC 4703 dwarf pair. We also detected star-forming regions along the
UGC 4703/ 4703B bridge with stellar mass exceeding 10$^{7}$ M$_{\odot}$. While
comparing the optical and HI morphology of the interacting dwarf pairs (UGC
4703-4703B and LMC-SMC) we discuss possible difference in interaction histories
of these systems.
