The galaxy presents as a disk galaxy, viewed at a high inclination, nearly edge-on. The galaxy exhibits a slight bulge. There appears to be a distinct separation between the disk and bulge. The galaxy displays a blueish hue on one side of the bulge and a orange hue on the other side of the bulge. The galaxy has a smooth, less-defined structure indicating older stellar populations and a relatively low star-formation rate. Evidence of a recent major merger is not apparent in the image; there appears to be no significant tidal distortions or other disturbances.
