The galaxy presents as a relatively faint, elongated structure with a high inclination, nearing edge-on. A bulge component is visible, and the concentration of light suggests it is largely spheroidal in nature, and appears to be rounded. The disk is visible, and appears relatively smooth. There are some hints of dust lanes within the disk, though the resolution limits definitive identification. There is no indication of a recent or ongoing major merger, though there appears to be some minor irregularity in the disk, which could be due to a minor interaction or internal processes. There appears to be some blue tint near the outskirts of the galaxy, suggesting ongoing star formation. 
