This galaxy exhibits a clear spiral structure. The spiral arms appear relatively well-defined, though somewhat flocculent. A central bulge is present; it appears of moderate size relative to the disk. The galaxy shows a slight inclination relative to our line of sight, as evidenced by the elliptical shape of the disk. Patches of bluer light are observable within the arms suggesting ongoing star formation. There appears to be a potential disturbance in the morphology, possibly indicating a minor interaction or tidal effect on one side of the galaxy. A bar structure appears present through the center of the bulge, it is difficult to tell the strength. The disk is not viewed edge on. There are no substantial dust lanes obviously visible.
