The galaxy presents as a spiral type, inclined at a high angle to our line of sight, but not quite edge-on. Two prominent spiral arms are tightly wound. A central bulge is visible, though of moderate size. The disk shows relatively smooth features, suggesting a lack of major ongoing mergers or disturbances, although minor disturbances may be present. The spiral arms show loose structures, extending fairly far out from the central bulge. There are no strong indications of a central bar feature. The galaxy's color suggests an intermediate population of stars, with moderate star formation activity.
