The galaxy presents an irregular morphology, suggesting it may be undergoing or have recently undergone a merging event. There are notable disturbances in the light distribution, indicating possible tidal features or ongoing interactions. While some regions appear relatively smooth, others show more complex structures, potentially containing disks or spiral arms. The color gradient suggests ongoing star formation, with bluer regions hinting at younger stellar populations. The galaxy is moderately luminous, with a significant portion of its light concentrated in the central region. There is evidence of substantial mass, potentially in the range expected for a typical galaxy. The presence of both relatively smooth and disturbed regions suggests a complex evolutionary history for this galaxy.
