The galaxy presents a spiral morphology, displaying prominent, loosely wound spiral arms. These arms appear somewhat clumpy and extend outwards from a central, moderately bright galactic bulge. The bulge appears relatively small in comparison to the disk. The galaxy exhibits a relatively face-on orientation. There is a suggestion of a possible bar structure in the central region. There appears to be no current major merger event, though there could be minor disturbances in the arms. The object possesses a blueish hue, suggesting active star formation in the disk.
