The galaxy appears to be undergoing a merger event. Two distinct, bright nuclei are visible within a common, distorted envelope of light. The overall shape is elongated, and neither nucleus exhibits a clear, undisturbed morphology. The light distribution between the nuclei suggests tidal interactions and potential star formation regions. The color is generally yellowish, potentially indicating an older stellar population, though regions of bluer light are present. No distinct spiral arm structure or prominent dust lanes are apparent. The morphology suggests that it is an interacting system well past initial contact.
