The galaxy appears to be a spiral galaxy with a prominent disk structure. While the galaxy is clearly not edge-on, it is not perfectly face-on either, but rather at a slight inclination relative to our line of sight. The galaxy exhibits well-defined spiral arms, which are tightly wound around the central bulge. The color suggests active star formation, particularly in the spiral arms, appearing as a bluer hue compared to the central bulge. There may be a slight bar structure. The bulge appears moderately sized. There does not appear to be any major disturbance or signs of a merging event.
