The object presents as a spiral galaxy. It appears to be at a slight angle to our line of sight, though not entirely edge-on. Two dominant spiral arms are clearly visible, extending from a central bulge. The winding of the spiral arms appears to be loose. There is a faint suggestion of a bar structure bisecting the central bulge. The color gradient suggests active star formation within the spiral arms, with bluer regions indicating younger stellar populations. There may be another galaxy merging with this galaxy or tidal debris from a past merger.
