The galaxy exhibits a spiral morphology with a relatively small bulge. The spiral arms are well-defined, displaying a relatively tight winding pattern. Two dominant spiral arms are clearly visible. The central bulge appears yellowish in color. The arms themselves show variations in color, possibly indicating regions of ongoing star formation, particularly in the outer regions of the disk. There appears to be a mild disturbance in the disk, perhaps the result of a small interaction. The galaxy appears relatively massive. 
