The galaxy presents as a spiral structure, exhibiting prominent, well-defined arms. The arms are tightly wound, suggesting a developed morphology. They originate from a central bulge that appears relatively compact, with a luminosity gradient from the center outward. The presence of distinct, resolved spiral arms indicates ongoing or recent star formation within the disk. The overall color suggests the presence of both older stellar populations in the central bulge and younger, bluer stars in the spiral arms. There are no apparent major disturbances or signs of an ongoing major merger event visible in this image, although a minor interaction cannot be ruled out. The disk of the galaxy is not seen edge-on. There may be the presence of a bar within the galaxy, however, it is difficult to discern any strong structures due to the resolution of the image. There seems to be the presence of two spiral arms. 
