This galaxy appears to be a disk galaxy viewed at a high inclination, nearly edge-on. There is a bright, concentrated central bulge. Dust lanes are visible, obscuring portions of the disk and suggesting significant dust content within the galaxy. The disk itself appears relatively smooth. There is potential evidence of a minor disturbance of the disc, possibly with tidal tails and/or distorted structures. This galaxy does not display a regular spiral structure. Overall, the galaxy is moderately luminous, with a relatively high surface brightness in the central region.
