This galaxy presents as a spiral type, with a prominent disk structure. The spiral arms appear loosely wound, exhibiting a flocculent morphology. Two distinct arms are discernible, extending outwards from a central bulge region. A bar structure is present, appearing somewhat weak and elongated through the center of the galaxy. The bulge appears moderate in size relative to the disk. The disk component is viewed at a somewhat tilted angle relative to our line of sight. There is no evidence of a major merger event. The disk exhibits varying degrees of star formation and is slightly disturbed.