The galaxy presents as a spiral type, with a disk-like morphology that is not oriented perfectly face-on. It exhibits a distinct central bulge region which appears yellow-orange in color, suggesting an older stellar population dominating this area. Two prominent spiral arms are observable emanating from the central bulge, winding loosely around the galaxy. The arms appear mottled, with variations in color indicating regions of differing star formation activity. Darker regions may be indicative of dust lanes within the spiral arms. There is little evidence to suggest ongoing major merging events or significant tidal disturbances in the system. The central bulge is of moderate size in relation to the disk of the galaxy. Evidence of a bar is seen across the central bulge of the galaxy. 
