This galaxy appears to be a spiral galaxy with a prominent disk. The disk is oriented at an angle relative to our line of sight, making it appear somewhat elongated, although there is a component that looks nearly edge-on. The central bulge is visible and appears yellowish. This suggests an older stellar population. The disk shows some indications of active star formation. There seems to be a recent major merger or significant tidal disturbance occurring with another galaxy, with disrupted spiral arms or tails extending from the main galactic body. The galaxy seems to be experiencing active star formation.
