The galaxy in the image presents as a spiral galaxy, exhibiting a clear disk structure. The spiral arms are readily visible, loosely wound around a central, brighter bulge region. The arm morphology indicates ongoing or recent star formation, identifiable by subtle blue hues. One arm appears to be more defined than the others. There is a possible tidal disturbance present, which may indicate an ongoing merger event, or a tidal interaction with a smaller galaxy. The core of the galaxy is not particularly defined; it may have a supermassive black hole or may not. There is an additional possible galaxy in the frame, but its qualities are hard to gauge. The overall structure suggests an actively evolving system, where gravitational dynamics and star formation processes are actively reshaping its appearance.
