The galaxy presents as a spiral with a disk-like structure. Evident spiral arms extend from a moderately sized central bulge, appearing relatively tightly wound. The color distribution suggests active star formation within the arms, evidenced by bluer hues, while the bulge exhibits a more yellow-white coloration, potentially indicating an older stellar population. There is no immediately apparent central bar structure. The galaxy displays only minor distortions, and there is no clear evidence of an ongoing major merger event. The spiral arm count seems difficult to precisely measure.
