The galaxy appears to be a spiral galaxy with a relatively small bulge. The spiral arms are loosely wound and defined, displaying a yellowish hue, indicative of an older stellar population within the arms. Two spiral arms can be seen, and there are no obvious signs of clumpy star formation. The galaxy disk is not edge-on. The central bulge region appears moderate in size, with a somewhat smoother texture compared to the arms. No strong bar structure is evident, with a possible weak bar. Indications show a likely galaxy merger or minor disturbance in the galaxy's structure.
