The galaxy presents a spiral morphology. Two distinct spiral arms are clearly visible, winding loosely from the central bulge. The spiral structure appears somewhat flocculent, lacking sharp definition. The central bulge exhibits a moderate size relative to the overall disk, appearing neither dominant nor negligible. There's some evidence of a weak bar structure in the central region, though not highly pronounced. The disk appears face-on relative to our line of sight. There is no apparent evidence of major mergers, but it does not appear to be a relaxed galaxy.
