The observed galaxy presents a complex morphology, exhibiting characteristics of both spiral and irregular types. The object appears to be largely disk-dominated, with no apparent bulge structure visible. The primary disk component is not smooth, but instead shows clumpy regions likely indicating areas of enhanced star formation. Traces of spiral arms are observed, although not as clearly defined.

There are indications of significant disturbances, suggesting a possible ongoing or recent merger event. Overall, the galaxy shows significant features, lacks a clear defined structure, and demonstrates possible merger activity.
