This galaxy presents as a highly inclined, edge-on spiral. A prominent dust lane is clearly visible, bisecting the galaxy along its major axis and obscuring the central bulge. The bulge appears to be relatively small and elongated, with a slight boxy appearance, and a yellow-white hue, suggestive of an older stellar population. The galactic disk shows distinct blue hues, especially towards its outer edges, indicating ongoing star formation activity. The disk appears smooth and undisturbed, showing no signs of major tidal interactions or recent mergers. The overall morphology suggests a relatively quiescent, well-established spiral structure.
