The galaxy appears to be a spiral galaxy, observed at an intermediate inclination angle. It has a noticeable central bulge that appears moderate in size, with spiral arms emerging from the central region. These arms appear somewhat loosely wound and possibly flocculent. There is evidence of active star formation within these arms, as indicated by the presence of bluer regions. The galaxy appears to be barred, however, it is not particularly strong. There are no signs of any major merging events occurring in the galaxy.
