The galaxy presents as a spiral galaxy, observed at a considerable tilt relative to our line of sight.  Spiral arm structure is evident, extending outwards from a central bulge. The arms appear somewhat patchy, with regions of bluer light suggestive of ongoing star formation.  The central bulge appears yellow-orange, indicating an older stellar population. The disk component dominates the overall structure. No significant bar structure is visible, and there are no obvious signs of ongoing merger activity or major morphological disturbances. The galaxy appears relatively isolated, without any nearby companions. 
