The galaxy appears to be an edge-on spiral galaxy. There is a prominent central bulge, which appears smooth and slightly elongated. A flattened disk extends outwards from this bulge and is oriented nearly parallel to our line of sight. The light distribution within the disk appears relatively uniform, but there are subtle color variations, with the central bulge being more yellow and the outer disk showing hints of bluer colors. Dust lanes are likely present obscuring some of the light from behind the galaxy within the disk and the disk appears asymmetrical. There are no obvious signs of a major ongoing merger, though there may be signs of a minor disturbance.