The galaxy presents as a face-on spiral type, exhibiting distinct spiral arm structures. These arms are not tightly wound, instead appearing relatively open. Within the spiral arms, there is evidence of active star formation regions, indicated by blue-ish concentrations, giving the arms a somewhat clumpy appearance. The galaxy possesses a noticeable central bulge, although it is not overly dominant in size, appearing moderate. The bulge region displays a smoother, more uniform color profile compared to the arms. There does not appear to be any edge-on disk component. There are some morphological disturbances and some evidence of weak tidal features, potentially indicative of an ongoing or past interaction/merger with a smaller galaxy. Based on the lack of any smooth appearance, there is no real evidence that this is an elliptical galaxy.
