The galaxy presents as a somewhat irregular spiral, exhibiting a moderately inclined disk structure. Evidence suggests possible ongoing or recent merger activity, characterized by disturbed morphology and areas of intense star formation, indicated by the clumpy, bluish regions spread throughout the galaxy. The central bulge appears relatively small and not very prominent, with no clear bar structure visible in this image. Overall, the galaxy displays a complex morphology, which points towards possible tidal interactions or internal dynamic processes. The spiral arms are not clearly defined but appear somewhat patchy.
