The galaxy displays a complex morphology, potentially indicative of a system undergoing a merger or significant interaction. A prominent feature is an elongated tidal tail extending from the main galactic body. There are at least three distinct bright knots present. These knots exhibit a greenish hue, suggesting regions of active star formation. The central region displays a redder color profile, potentially indicating an older stellar population or a higher dust content attenuating bluer wavelengths. There is some distortion present in the main galactic body, potentially related to gravitational disturbances. Overall, the galaxy appears to be actively evolving.
