This galaxy appears to be undergoing a significant interaction, possibly a merger. It presents a complex morphology, showing signs of disturbance rather than a well-defined structure. There is evidence of tidal features extending away from the main body, suggesting gravitational disruption due to the interaction. A component of the object is smooth in appearance, possibly an older stellar population. The galaxy emits strongly in the blue, green, and red portions of the spectrum, suggesting it has ongoing star formation. The overall color is on the redder side, potentially indicative of a significant population of older stars in addition to regions of more recent star formation.
