The galaxy presents as a disturbed system, exhibiting characteristics suggestive of a merger event. The overall morphology is irregular, lacking a well-defined structure. Two distinct, bright nuclei are apparent, indicating the presence of at least two galaxies in close interaction. Tidal features, such as faint stellar streams or tails, are observed extending outward from the main body of the galaxy, further supporting the merger hypothesis. The color distribution is heterogeneous, with bluer regions potentially indicating areas of active star formation, while redder regions may correspond to older stellar populations. The system does not appear to be an edge on disk galaxy, but more likely an irregular shape. The lack of clear spiral arms suggests a system in a relatively late stage of merging, where the original galactic structures have been significantly disrupted. There may be possible dust lanes obscuring some star formation regions.
