The galaxy appears to be a spiral, although the arm structure is not well-defined. The central bulge is prominent and shows a slightly yellowish-white hue, suggesting an older stellar population. Extending outward from the bulge is a disk, exhibiting a blueish tint that indicates the presence of younger, hotter stars. The overall shape of the galaxy is elongated, but there is some indication that it could also be an edge-on disk galaxy. There may be some signs of minor disturbances within the disk, but no large scale disruptions appear to be present.
