The observed galaxy presents as a spiral galaxy viewed at a high inclination, approaching edge-on. The galactic disk is the dominant feature, exhibiting a bluish hue indicative of active star formation. Two loosely wound spiral arms are present extending away from the central bulge. The bulge appears small in proportion to the overall size of the galaxy, but is well defined. There is a moderate bar present. The presence of a tail indicates there is minor disturbance due to gravitational effects from a tidal interaction or recent minor merger.
