The galaxy presents as a relatively faint, edge-on or highly inclined disk galaxy. It exhibits a somewhat elongated shape, consistent with a flattened disk structure viewed at an angle. There is a subtle color gradient visible across the galaxy's extent, suggestive of varying stellar populations or dust distribution. The central region is subtly brighter compared to the outer regions, perhaps indicating a concentration of older stars. There is some evidence of patchy light distribution along the disk, hinting at the presence of spiral arm structures, or regions of active star formation. The overall blueish hue suggests the presence of young, hot stars, although the galaxy isn't exceptionally bright, and may be quiescent with low rates of current star formation. There appears to be some slight asymmetry along the galactic plane, suggesting possible interactions or disturbances in the past. The morphology does not show any obvious signs of a recent major merger, but minor disturbances cannot be ruled out based on this image.
