The galaxy appears to be a spiral galaxy, viewed at a slight incline relative to face-on. The spiral arms are readily apparent and show a winding intermediate between tightly wound and loosely wound. Faint indications of a possible bar structure are present within the central region. The galaxy possesses a distinct bulge component of moderate size, although the bulge may not be the dominant morphological feature. A possible disturbance in the galaxy's morphology exists, although whether this is a minor disturbance, major disturbance, or possible merger with another galaxy is uncertain. The disk is the most noticeable feature.
