The object appears to be a spiral galaxy, viewed at a slight angle relative to face-on.  The spiral arms are not tightly wound but rather present a more open, grand-design structure. A central bulge is visible, and the rest of the galaxy appears moderately bright.  The arms appear somewhat flocculent, with a subtle blue color, especially in the outer regions. The object's disk shows hints of ongoing star formation.  There is no obvious sign of strong gravitational disturbance or a major merger.
