This galaxy appears to be a spiral galaxy, seen at a slight incline relative to our line of sight. The disk shows defined spiral arm structures. These arms exhibit a patchy distribution of light, suggesting active star formation regions. There is a moderate central bulge that is a prominent feature. The disk dominates the overall light profile. The galaxy does not exhibit a bar structure. There appear to be no major signs of ongoing merger activity or strong gravitational disturbance. The colour is dominated by blue light.
