The galaxy presents as a relatively smooth and elongated structure. It exhibits a central concentration of light, but there are no distinct spiral arms or a prominent bulge visible. The overall color is predominantly bluish, suggesting the presence of a younger stellar population. The galaxy's shape is somewhat cigar-like, with a major axis clearly longer than its minor axis. There is no obvious evidence of major mergers or significant tidal disturbances, although minor disturbances are not completely ruled out.
