The galaxy appears to be an edge-on spiral or lenticular galaxy, with a notable central bulge that seems to be relatively large and has a rounded shape. There is a disk component to the galaxy, however, it is difficult to discern any distinct spiral arm structure from this viewing angle. The disk appears to be smooth and somewhat featureless, although some subtle variations in color suggest dust lanes or regions of differing stellar populations. The overall color of the galaxy is somewhat redder than expected in comparison to typical spiral galaxies, perhaps indicating an older stellar population or significant dust obscuration. There is no obvious evidence of a major ongoing merger event, but there are some subtle asymmetries in the galaxy's structure and potential signs of a minor disturbance, particularly in the outer regions of the disk.
