This galaxy presents as a disk galaxy, viewed edge-on from our line of sight. The central bulge exhibits a prominent, rounded morphology with a high degree of symmetry. Dust lanes appear to be obscuring the central bulge, but it may also be comprised of older stellar populations, giving it a yellowish hue. The disk of the galaxy shows some indications of slight disturbance, but is primarily a smooth appearance, but there is a slight warp to it. There are hints of faint spiral structure along the edges of the disk. Overall, the galaxy is experiencing relatively low star formation activity, with most activity concentrated in the central bulge.
