The galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent merger event. Two distinct components appear to be interacting, displaying tidal features and disrupted structures. The primary component shows a hint of a disk-like structure, although it is heavily distorted. The second component is smaller and more amorphous in shape. Overall, the system presents with moderate star formation activity, indicated by the mixed population of younger and older stars. The galaxy emits light across a broad spectrum, with stronger emission in the redder bands, indicating a significant population of evolved stars. The estimated size of the galaxy is approximately 13 kpc.
