The galaxy appears to be a spiral galaxy viewed edge-on. A prominent dust lane bisects the galaxy, obscuring the central bulge region. The bulge presents a round morphology. The disk component is readily apparent as a linear structure, with a color gradient that shows a bluer tone towards the outer reaches. The light from the disk appears asymmetric, implying a warped structure or uneven distribution of stellar populations. There are no readily visible signs of ongoing major mergers, although subtle perturbations within the disk may indicate past minor interactions. 
