The galaxy presents as a relatively smooth, disk-like structure, viewed at a significant inclination. The central region exhibits a higher surface brightness, possibly indicative of a bulge component. The disk shows a subtle color gradient, with a somewhat bluer hue towards the outer regions, suggesting the presence of younger stellar populations or ongoing star formation within the disk. There are no obvious signs of strong spiral arms or significant dust lanes. The overall morphology suggests a late-type spiral galaxy, although the smoothness could also imply a lenticular galaxy. There appears to be a slight asymmetry in the outer regions, possibly due to a minor gravitational interaction or past merger event, but generally appears undisturbed.
