The galaxy exhibits a spiral structure with a moderate inclination relative to our line of sight. Spiral arms are discernible, though somewhat flocculent in appearance, and extend from a central bulge region. The bulge is relatively small compared to the overall size of the galaxy. Evidence of dust lanes is present within the spiral arms, and they appear to be tightly wound. The overall color is slightly blue, suggesting the presence of relatively young stars and ongoing star formation. There are no obvious signs of major interactions or mergers, though there might be some minor disturbances. Bar structure is either not present or indistinct.