The object is a spiral galaxy, viewed at a slight angle from face-on. The central bulge is a bright, yellowish hue and appears moderately sized, gradually fading out into the disk. The spiral arms appear tightly wound, extending outward from the bulge. The color of the spiral arms is predominantly bluish, suggesting active star formation. There may be more than two spiral arms, but the exact number is difficult to determine due to the moderate winding and image resolution. There is no noticeable central bar structure present within the galaxy. The disk displays some degree of irregularity, possibly due to minor gravitational disturbances. There is no evidence of a major merger currently taking place.
