The galaxy presents as a spiral type, viewed at a considerable inclination, approaching edge-on. The disk appears prominent. The central bulge region is notable, exhibiting a bright, concentrated luminosity. A faint bar structure may be present across the center. Spiral arms are visible, extending from the central region. The arms appear somewhat clumpy. There is a slight asymmetry in the outer regions. A potential merger or tidal interaction may have occurred or be on-going.
