The galaxy presents a spiral morphology. Spiral arms are clearly visible, though somewhat flocculent. The color suggests a relatively high rate of star formation, particularly within the spiral arms. The central bulge appears moderate in size and a yellow-orange hue, implying an older stellar population as compared to the arms. The galaxy does not appear to be undergoing any major merging activity. There may be a faint, weak bar structure. There is a clearly defined disk.
