This galaxy exhibits a clear spiral structure. The spiral arms are readily apparent, displaying a moderate degree of winding. The central bulge appears moderate in size, with no obvious bar feature. The colouration is bluer in the disc compared to the bulge, and the surface brightness profile decreases smoothly outwards. The galaxy appears relatively undisturbed, showing no signs of major merging activity. The dust lanes seem less pronounced in comparison to the disk, and show evidence for present star formation activity.
