The galaxy presents as a spiral with a prominent disk structure. The disk is not perfectly edge-on, exhibiting some inclination. The spiral arms appear somewhat flocculent, with moderate winding. Two prominent spiral arms are observed. There are possible indications of substructure or star-forming regions within these arms. A central bulge appears, possibly moderate in size relative to the disk. There's no apparent strong bar structure. Overall, there might be some evidence of a minor disturbance or interaction but, the galaxy seems relatively isolated and unperturbed.
