This galaxy presents a predominantly edge-on disk orientation. A distinct bulge is not apparent; the light appears relatively uniform across the major axis. The color is strongly suggestive of an older stellar population. The galaxy exhibits a somewhat disturbed morphology, with asymmetry visible along its length. Some of this asymmetry could be caused by minor tidal disturbances. The overall color and smooth appearance suggest that it is a late-type galaxy with ongoing, but not particularly intense, star formation.
