The galaxy appears to be a spiral galaxy, though its morphology is somewhat disturbed. It exhibits a relatively faint, diffuse disk with a central, brighter bulge. There is a possible indication of a tidal tail extending vertically from the primary galactic disk. The color distribution suggests active star formation, with a greater concentration of blue-ish hues concentrated in the disk and potential star forming knots within the tail. Some indication of dust lanes may be present along the disk, however, high disturbance levels may be confounding a clear observation of the object.
