The galaxy presents a prominent disk-like structure, oriented at a slight angle to our line of sight. Spiral arms are clearly visible. These arms appear to be relatively well-defined. I observe two dominant arms. There seems to be some degree of asymmetry or disturbance in the outer regions of the disk. It appears to have a bar structure in the center. The galaxy exhibits a moderately sized bulge. The winding of the spiral arms seems to be of medium tightness. Finally, there is evidence of minor disturbances.
