The galaxy presents as a spiral, with a disk-like structure. Its orientation is nearly edge-on, obscuring a clear view of its central bulge. Faint, loosely wound spiral arms emanate from the central region and are easily seen as a blue hue. There appears to be a bar-like feature extending across the central region. There is no apparent major disturbance indicative of ongoing major merging activity, although some minor disturbances are possibly occurring. The galaxy appears to be of moderate mass and exhibits signs of star formation.
