The galaxy appears to be an edge-on spiral galaxy with a prominent central bulge. The bulge exhibits a smooth, concentrated light profile, suggesting a high stellar density. The disk is narrow and elongated, displaying some evidence of dust lanes, which attenuate the light and create darker regions along the plane. The overall color of the bulge appears more yellow/red than the rest of the disk, potentially due to older stellar populations. There is some evidence of recent star formation occurring with the disk region. There appear to be no close interacting bodies with the galaxy.
