The galaxy presents as an edge-on spiral with a prominent, centrally concentrated bulge. The bulge appears to be smoothly rounded. The disk is highly inclined, nearly perpendicular to our line of sight. Evidence suggests a high probability of a disk structure.

There is indication of an interaction or merger, as there are is evidence of some morphological disturbance, such as tidal features that may be the result of a recent merger. There seems to be possible additional objects involved, however it is difficult to distinguish given the image resolution.
