The galaxy presents as a flattened, disk-like structure seen nearly edge-on. A central bulge is subtly visible as a slightly brighter, more concentrated region. The disk shows a relatively smooth texture with a blue hue, suggestive of ongoing star formation. The light distribution is asymmetric, with one side of the disk appearing more extended and diffuse than the other. There's no strong evidence of spiral arms or significant dust lanes. There might be a very slight tidal disruption of the galaxy; however, it could be background noise from the instrument used to capture the image.
