The galaxy presents as a relatively well-defined spiral structure, although the arms appear somewhat flocculent. Its morphology is disk-dominated. The bulge appears moderate in size, exhibiting a concentrated central brightness which gradually diffuses outwards. A notable blue hue is present in the disk, suggesting active star formation. The galaxy is oriented with a high inclination relative to our line of sight. There is no immediately apparent distortion indicating a major merger event, however the galaxy does have more than two spiral arms.
