  We present visible and near-infrared images of the amorphous dwarf galaxy NGC
1705 in the $B$, $V$, $R$, $J$, $H$, and $K$ bands. Optical and near infrared
colors in the galaxy are consistent with a composite population with colors
similar to those of the bluest Sc nuclei. The contribution of young stars to
the disk population of the galaxy decreases outwards from the center. In the
near infrared images we detect three unresolved point sources, two of which
have colors and luminosities comparable to intermediate age LMC clusters.
