The galaxy presents as a spiral with a prominent disk and moderate bulge. The disk is oriented approximately edge-on, though not perfectly, allowing for some structure to be observed. The spiral arms are tightly wound and two-armed, with some regions displaying bluer hues suggestive of active star formation. The central bulge appears yellowish. There are no significant signs of major mergers or disturbances; any merging influence would be mild. The bar is present and may be slightly weak. There is some dust obscuration, but not too excessive.
