The galaxy appears to be a spiral galaxy, seen at an oblique angle. It has a prominent central bulge with a yellowish hue. The disk appears relatively smooth, with a suggestion of spiral arms, but the resolution limits a definite confirmation. Some bluer regions may be present within the disk, potentially indicating areas of ongoing star formation. There are hints of a dusty disk obscuring some of the light from the bulge. It shows no obvious signs of a major merger but slight visual disturbances can not be ruled out. The galaxy's light profile is elongated, indicative of its flattened shape.
