The galaxy presents as an elongated, edge-on spiral. A central bulge is visible, with a morphology that appears largely rounded. There is no strong evidence of a boxy morphology to the bulge. The disk component exhibits a relatively smooth texture. There is no strong visual indication of spiral arm structure within the disk, but the slight variations in color within the galaxy suggest internal features. The galaxy shows no obvious signs of a major merger event. There is also no major disturbance, nor a clear merging of the galaxy with another. It is likely that this is a regular galaxy, though there are subtle disturbances that are visible. The size and shape of the galaxy suggest that it may be disk-shaped.
