The galaxy presents a clear spiral morphology, exhibiting two prominent, well-defined spiral arms. The arms appear somewhat flocculent, showing distinct regions of enhanced star formation activity as evidenced by their bluer coloration. The galaxy has a notable bulge of moderate size, appearing yellowish-white, indicating an older stellar population.

Evidence suggests this galaxy is currently undergoing a merging event, as the morphology appears disturbed. There is another galaxy in contact with this galaxy, and both appear significantly disturbed. There are no strong indications of a bar structure within the galaxy's central region. The galaxy does not appear to be viewed edge-on.
