The galaxy presents a disk-like morphology, viewed at a slight inclination. Evidence of spiral arm structure is apparent, although the arms appear somewhat flocculent and not sharply defined. Two major arms appear to be visible, perhaps with several more minor ones present, though it is somewhat hard to count them due to the resolution. A central bulge is visible with a smooth appearance and a yellowish hue, suggesting an older stellar population in this region. The disk shows a bluer color profile, indicative of ongoing star formation. There is a subtle indication of a bar-like structure in the galactic center. The galaxy does not appear to be undergoing any major mergers or interactions, though it is quite difficult to say with absolute certainty.
