The galaxy presents as a moderately sized, somewhat disturbed system. It exhibits a flattened, disk-like structure, although its morphology appears significantly perturbed. There are no prominent spiral arms visible. The galaxy's light profile suggests a non-uniform distribution of stellar populations. We observe indications of an ongoing or recent merger event, evidenced by a disturbed morphology. Based on the color, there is evidence of at least some current star formation, but it doesn't appear particularly active.
