The galaxy presents as a spiral type, with a prominent, moderately sized bulge that is noticeably yellow in color. Spiral arms are clearly visible, extending from the central bulge. The arms are somewhat loosely wound and appear to exhibit a two-armed structure. The color of the spiral arms shifts toward blue, suggestive of ongoing star formation. There is no obvious bar structure visible in the central region. Based on the irregular light distribution within the arms, there may be minor disturbances due to gravitational interactions, but no major merger events appear to be occurring. The galaxy is neither a purely smooth elliptical, nor an entirely edge-on disk, possessing both disk and bulge components.
