The galaxy presents as a spiral type, observed at a slight angle from face-on. It exhibits a prominent central bulge that appears bright and concentrated, indicative of a high stellar density in that region.  

Two clearly defined spiral arms are visible, tightly wound around the central bulge. These arms show a distinct blue hue, possibly indicating active star formation regions within them.  There is also a strong bar-like structure running through the central bulge. The overall shape is generally ordered, though there are some hints of minor disturbances or asymmetries in the outer regions of the disk. 

