The galaxy presents as an edge-on spiral system. Its overall morphology suggests a flattened disk-like structure. A central bulge is present, with a moderate concentration of light. There appears to be some dust lane obscuration along the equatorial plane, evidenced by a slight color variation within the galaxy's disk. The galaxy exhibits a blueish color, which could be due to it's star forming properties. No signs of tidal disturbances or ongoing major mergers are immediately apparent, however minor disturbances may be present in the disk. The shape of the bulge appears to be more rounded than boxy.
