The galaxy exhibits a spiral structure, although it appears somewhat diffuse. Two distinct spiral arms emerge from a central region. These arms seem loosely wound. There are some regions of increased blue light within the spiral arms which likely indicates areas of increased recent star formation. The central bulge is small relative to the overall galaxy. There is likely gas and dust throughout the galaxy. The overall color suggests that the galaxy contains a mix of stellar populations. The galaxy does not appear to be highly inclined, but rather close to face on.
