The galaxy appears to be a spiral type, characterized by a prominent disk structure. The arms are well-defined and appear tightly wound around a central bulge. There appears to be two distinct spiral arms emanating from the central region. A bar structure is weakly indicated. The central bulge seems moderate in size relative to the overall galactic disk. There is no obvious visual indication of a major merger event. It is not an edge-on galaxy. The galaxy exhibits a smooth feature fraction.
