This galaxy presents as a spiral type, exhibiting well-defined spiral arms extending from a prominent central bulge. The arms appear to be traced by regions of star formation, indicated by the slightly bluer color, and dust lanes which can be seen crossing the arms. Two spiral arms are clearly visible, each extending approximately 180 degrees from their points of origin. The tightness of the spiral arms ranges from tight to loose. 

A bar-like structure appears to traverse the central bulge. The central bulge exhibits a moderate size, with a slightly yellow coloration, possibly indicating an older stellar population. There are indications of a minor disturbance or a merging event; there appears to be material pulled away from the main galactic disc.
