The galaxy presents a relatively smooth and centrally concentrated appearance. It exhibits a flattened, disk-like morphology, oriented approximately edge-on with respect to our line of sight. There is evidence of a bulge component. Some minor dust lanes are visible obscuring the central regions of the disk, most prominent along the equatorial plane. The overall colour is predominantly redder, indicative of an older stellar population and a relatively low current rate of star formation. There are hints of spiral structure, though it appears tightly wound and rather indistinct. No major signs of recent or ongoing merger activity are readily apparent.
