The galaxy presents as a spiral type, with a dominant disk structure. The spiral arms appear tightly wound around the central bulge. There may be a bar structure within the central region, though it is not highly pronounced. The bulge component is relatively small compared to the overall size of the disk. Star formation appears to be occurring within the spiral arms. There is no evidence of any major merging events or significant disturbances to the galaxy's morphology. There are subtle traces of red possibly indicating slight dust lanes or regions of older stellar populations within the disk. The overall color suggests a mix of stellar populations, with a slightly bluer hue in the outer regions, and yellower color in the inner regions indicating a greater population of old stars.