The galaxy presents a spiral morphology, exhibiting a disk-like structure with tightly wound spiral arms. The arms are not uniformly distributed, but are clearly distinguished and extend outwards from a central bulge. The bulge appears to be moderate in size. The overall color of the galaxy suggests a mix of stellar populations, with bluer hues along the spiral arms potentially indicating younger, hotter stars and active star formation, compared to the yellowish color towards the center. There is a second object visible, potentially interacting, but its appearance suggests it is most likely a background object or companion galaxy. The galaxy is viewed at an oblique angle, neither face-on nor edge-on. No significant signs of recent major merging activity are evident, although some minor disturbances in the morphology cannot be ruled out based on this image alone. There also appears to be a bar.
