This galaxy presents a complex morphology, appearing disturbed and potentially undergoing a merger. The central region exhibits a relatively smooth profile, with an overall elliptical shape. There is evidence of a prominent, irregular structure that dominates a significant portion of the galaxy. The light distribution is not uniform, showing patches of varying intensity. Colors appear bluer in parts of the extended structure and redder in other regions. Overall, the galaxy has an estimated effective radius on the order of a few kiloparsecs. The image shows disturbances that indicates a moderate degree of star formation, but the presence of a smooth central component suggests that the central region could be composed of an older stellar population.
