The galaxy presents a disk-like morphology, viewed at an inclined angle, which reveals a rich, complex structure. Spiral arms are apparent, exhibiting a winding pattern that transitions from tightly wound in the inner regions to more open in the outer arms. The galaxy displays evidence of active star formation regions, particularly along the spiral arms, indicated by the presence of blue light, indicative of hot, young stars. The central region hosts a bright, concentrated bulge, although it does not appear to dominate the overall light profile of the galaxy. There seems to be no distinct bar structure. There is a slight possibility that it is interacting with another galaxy, as the edges are not defined cleanly.
