The galaxy presents as a spiral structure viewed approximately face-on. The central bulge appears relatively small and diffuse, with a moderate contribution to the overall galaxy luminosity. The spiral arms are tightly wound and extend outwards from the central region. There is evidence of active star formation within the spiral arms, indicated by their bluer color, with more amorphous regions indicating areas of lower concentration of stars. The disk is the dominant structural component of the galaxy, with no apparent bar feature visible in the central region. The overall morphology is largely undisturbed, exhibiting no signs of a recent major merger event, although there may be some minor interaction present that is causing distortion of the arms..
