The galaxy presents as a grand design spiral. The central bulge appears moderate in size with a bright core. Two distinct spiral arms are present, winding moderately around the central bulge. The arms appear somewhat patchy in color and structure, suggesting regions of active star formation. The overall disk is not perfectly face-on, showing a slight inclination. No major signs of ongoing merger activity are evident, though minor disturbances within the spiral arms cannot be ruled out. A weak bar structure might be present in the central region, based on a slightly elongated shape, but it is not definitively clear. The galaxy is relatively isolated.
