The galaxy presents as a late-type spiral with ongoing merger activity. The spiral arms are well-defined but appear significantly distorted, indicating a possible interaction with another galaxy. There is a notable tidal tail structure extending from one side of the galaxy. The central bulge is moderately sized and appears yellow in color suggesting an older stellar population, but is not distinct. The disk exhibits a blue hue, indicative of more recent star formation activity. There is a clear asymmetry in the light distribution across the galaxy, possibly as a result of the merging event. The galaxy exhibits features consistent with a major merger, displaying strong tidal features and a disturbed morphology. It is unlikely that this is an edge-on disk. The evidence suggests ongoing gravitational interaction is substantially impacting the galaxy's morphology and star formation.
