The object appears to be a spiral galaxy, observed at an angle that is tilted relative to our line of sight. The spiral arms are prominent, with a loose winding pattern and a possible two-arm structure. The central bulge is noticeable, appearing as a distinct component, but does not dominate the overall structure. There are some potential signs of tidal distortions, suggesting either a minor or major disturbance within the galaxy. The arms themselves display variations in color and brightness, possibly indicating regions of active star formation within them.
