The galaxy presents as a relatively small, faint, edge-on spiral system. A distinct dust lane bisects the galaxy along its major axis, obscuring the central bulge. The bulge appears prominent and is elongated along the plane of the disk. The central region exhibits a yellow-orange hue which may suggest an older stellar population. Hints of bluer light are observed surrounding the bulge which may point to some ongoing or recent star formation. There is no evidence of any tidal features, suggesting that the galaxy has not recently undergone a major merger.
