The galaxy presents as a disk galaxy, observed at a high inclination, nearly edge-on. There is a prominent central bulge, exhibiting a relatively smooth, concentrated morphology. The disk component displays a yellowish hue, possibly indicative of an older stellar population with lower levels of recent star formation. There may be some level of disturbance in the disk, as there appears to be slight warp or asymmetry. The galaxy appears to be a relatively massive system.
