The galaxy presents as a relatively faint, edge-on spiral. A prominent dust lane bisects the galaxy along its major axis, obscuring a significant portion of the central bulge. The bulge appears to be rounded rather than boxy. The disk is visible but not well-resolved, lacking distinct spiral arm structures in the available image resolution. The galaxy shows no strong visual signs of major interactions or mergers, although a minor disturbance cannot be ruled out. There is a small nearby galaxy that is clearly seen with is own morphology. The galactic disk is characterized by a smooth distribution of light, which may be indicative of ongoing, albeit not exceptionally high, star formation.
