The galaxy presents as a spiral type, exhibiting a distinct disk structure. The spiral arms are well-defined and appear tightly wound around a central bulge. The bulge component is relatively prominent, yet appears moderate in size, compared to the entire galaxy. The galaxy displays a primarily face-on orientation.

Evidence suggests current or recent star formation is present, noted by the blue color evident in the spiral arms and the overall morphology of the disk. There do not appear to be signs of major interaction or disturbance in the immediate vicinity of the galaxy. The general structure suggests a gravitationally stable system.
