The galaxy presents as a relatively smooth, centrally concentrated object with a flattened, disk-like structure. It exhibits a prominent bulge that appears nearly spherical. The bulge displays a yellowish color, suggesting an older stellar population. Moving outwards from the bulge, the disk becomes visible, displaying a bluer hue indicative of younger, hotter stars. The disk does not show well-defined spiral arms or distinct features, it has a subtle fuzziness to it. The general shape of the galaxy appears between elliptical and a highly inclined spiral. There seems to be a very minor disturbance of some kind, the light appears uneven. The overall light profile suggests a system undergoing a period of relative quiescence with moderate, but low, levels of star formation.