The galaxy appears to be a spiral galaxy, viewed at an oblique angle, but with a distinct disk structure. The disk shows evidence of spiral arm structure. There is a strong central bar feature, which is unusually bright and clearly visible. The bulge component appears relatively small. The galaxy shows no clear signs of a major merger or significant tidal disturbances. The bluer color on the outer edges and along the spiral arms hints at ongoing star formation. The relatively high degree of organization suggests this is not a recently merged system.
