The galaxy exhibits a somewhat elongated, irregular morphology. A significant portion of the galaxy appears relatively smooth and featureless, but with a clumpy appearance. There is evidence of a disk-like structure, and some disturbance. The color distribution suggests a mix of stellar populations, with some regions exhibiting bluer hues, potentially indicating ongoing star formation, and other regions that are redder. The presence of any large tidal features is not apparent. It could possibly be an interacting galaxy as it is a bit disturbed.
