The galaxy presents as an edge-on spiral, or possibly lenticular, galaxy. Its morphology suggests a disk-dominated system. A blue hue permeates the galaxy's disk, indicative of ongoing or recent star formation activity. Two localized bright regions, possibly associated with star-forming regions, are discernible along the disk. Dust lanes are subtle or absent; the disk is relatively smooth with only minor disturbances to the overall structure. The central bulge is ill defined and blended with the disk and the light tapers off quickly, the galaxy is very diffuse.
