The galaxy presents as a disturbed system, possibly interacting with another galaxy. It exhibits a notable tidal tail, or bridge of stars, extending from the main body, suggesting gravitational interaction. The main body of the galaxy appears distorted, lacking a clear spiral or elliptical structure. There is evidence of active star formation, indicated by the greenish hue. The core regions show a redder color, indicative of an older stellar population. The galaxy is moderately bright, displaying a well-defined disk structure, although distorted. The overall morphology suggests a system undergoing a merger or close interaction, leading to the observed tidal features and irregular shape.
