The object is a spiral galaxy, presenting a tilted orientation relative to our line of sight. The galaxy exhibits a prominent central bulge. Faint spiral arms emanate from the bulge, extending into the outer regions of the galaxy. The spiral arms are not tightly wound but appear somewhat dispersed. The disk component shows a bluer hue. There may be some minor disturbances within the galaxy, but no major indications of merging activity can be determined from the image. The core of the galaxy is a yellowish-green hue.
