The galaxy presents as a spiral, with tightly wound arms emanating from a prominent central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. The spiral arms appear flocculent, with variations in brightness and color indicating ongoing star formation regions interspersed with dust lanes. The disk of the galaxy is tilted with respect to our line of sight, presenting an oval shape. There appears to be a strong central bar bisecting the bulge, and its orientation is approximately vertical in the image. Some degree of asymmetry or minor disturbance appears present in the outer regions of the disk. The galaxy appears relatively isolated.
