The galaxy presents as a disk galaxy, viewed at a moderate inclination. There is evidence of spiral arm structure, though it is somewhat flocculent and ill-defined. A central bar structure appears to be present across the galaxy’s core. A bulge appears to be significant and dominates the core region of the galaxy. The bulge contributes substantially to the galaxy's overall luminosity. No major mergers are clearly visible in the image, but there appears to be some minor disturbance in the disk.
