The galaxy presents as an edge-on spiral, displaying a high degree of inclination relative to the observer's line of sight. A prominent dust lane is visible, bisecting the galactic disk and obscuring a significant portion of the starlight. The bulge appears elongated and primarily rounded, not showing any obvious boxy features. The disk exhibits a faint and somewhat diffuse structure, appearing relatively smooth. Hints of disturbances or minor irregularities are visible, but no major merger event is indicated, nor does it display significant star formation activity. Overall, the galaxy presents as relatively massive.
