This galaxy presents as a disk galaxy, viewed approximately edge-on from our vantage point. The primary structure is a flattened, elongated form with a brighter central bulge. There is a subtle lane of obscuration visible along the central plane, suggesting the presence of dust and gas within the galactic disk.

The overall color of the galaxy appears to be dominated by bluer wavelengths, particularly in the extended disk region. This might indicate ongoing star formation in this area. The central bulge appears more neutral in color, possibly implying an older stellar population.

There appears to be a minor gravitational disturbance or interaction occurring, as suggested by a slight asymmetry or warping in the disk's morphology. This disturbance could be the result of a previous or ongoing minor merger event.
