The galaxy appears to be a spiral galaxy, viewed at a significant angle, nearly edge-on. The central bulge is prominent and appears yellowish-orange in color, suggesting an older stellar population. A disk component is visible, extending away from the bulge. There is a slight blue tint to the far edges of this galaxy. The disk appears relatively smooth, without obvious strong spiral arm features. This galaxy is potentially a minor merger or experiencing some sort of gravitational disturbance.
