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We present visible and near-infrared images of the amorphous dwarf galaxy NGC1705 in the $B$, $V$, $R$, $J$, $H$, and $K$ bands. Optical and near infraredcolors in the galaxy are consistent with a composite population with colorssimilar to those of the bluest Sc nuclei. The contribution of young stars tothe disk population of the galaxy decreases outwards from the center. In thenear infrared images we detect three unresolved point sources, two of whichhave colors and luminosities comparable to intermediate age LMC clusters.Comment: uuencoded compressed tarred postscript including figures. Accepted  for publication in AJ

The Dwarf Galaxy NGC 1705-A Highly Composite Stellar Population