The galaxy appears as a highly inclined disk galaxy, viewed nearly edge-on. There is a prominent dust lane visible, bisecting the galaxy's luminous profile along its major axis. The central bulge is moderately pronounced and appears rounded. The galaxy exhibits a smooth, elongated morphology with a gradual fading of light intensity from the center towards the outer edges. Faint color variations are discernible across the disk, suggestive of differing stellar populations. There are no signs of major disturbances or ongoing mergers, although subtle asymmetries in the outer disk regions might indicate minor gravitational interactions. The overall structure is largely undisturbed and presents a classic edge-on disk galaxy configuration.
