This galaxy appears to be a spiral type, viewed at an oblique angle. The spiral arms are somewhat flocculent, with regions of increased stellar density visible within them. A central bulge is present, with a moderate amount of light concentrated within it. The disk of the galaxy exhibits a blue hue. A bar feature is visible, appearing to extend through the galactic center. There are signs of a possible interaction or merger event. The galaxy exhibits irregular features with some evidence of tidal tails or distorted morphology. 
