This galaxy appears to be a spiral galaxy, observed nearly edge-on. A prominent central bulge is visible, with a moderate degree of boxiness. The disk of the galaxy is highly inclined relative to our line of sight, with little to no arm structure immediately visible. There is evidence of dust lanes present within the disk. The galaxy exhibits a gradient in color, with the bulge appearing more red/orange. The disk has a bluer component. The overall structure appears relatively undisturbed, suggesting the absence of recent major mergers. 
