The galaxy presents as an elongated structure, consistent with a disk galaxy viewed at a significant inclination. The galactic profile appears relatively smooth and featureless. There is no prominent central bulge. The colors within the disk appear generally uniform, suggestive of an older stellar population with less ongoing star formation. There is no apparent dust lane. There are no signs of any major disturbances or ongoing mergers. It appears to be an isolated galaxy without close companions in the immediate field of view.
