The observed galaxy appears to be a spiral galaxy viewed edge-on. A prominent dust lane is visible, bisecting the galaxy's disk and obscuring a significant portion of its central bulge. The bulge exhibits a relatively smooth, rounded morphology. Faint disk structures are visible extending from the bulge, indicating the presence of stellar populations within the galactic plane. Based on the color distribution, it appears that the galactic bulge is dominated by older stars, and disk appears to have regions of star formation occurring. The galaxy's overall structure suggests it is relatively undisturbed, without major signs of tidal interactions or ongoing mergers.
