This galaxy presents as a disk galaxy observed nearly edge-on. There is a central bulge, elongated and relatively smooth in appearance, though it is more boxy in shape than elliptical. Faint spiral arms appear to be present, with a dusty band visible that obscures some of the bulge. There is no evidence of a recent major merger; however, minor disturbances are present. Based on the color, we can speculate that this galaxy is relatively mature with an intermediate mass, and a very low specific star formation rate.
