The galaxy presents as a spiral structure viewed at a relatively low inclination angle. Two distinct spiral arms are discernible, loosely wound and emanating from a somewhat obscured central bulge region. The bulge appears yellowish in color, suggesting a population of older stars. The spiral arms exhibit a bluer hue, indicative of ongoing star formation. There is an indication of some dust lane presence within the spiral arms, but not very prominent. There is no visible bar structure. The overall morphology suggests a galaxy undergoing active star formation within its spiral arms. There may be some minor disturbance.
