The galaxy presents as an edge-on spiral, likely a disk galaxy. The prominent dust lane bisecting the galaxy is indicative of this morphology. The central bulge appears substantial and exhibits a more yellow to golden hue, suggesting an older stellar population. The disk itself displays a bluer color, hinting at ongoing star formation within its spiral arms, though the limited resolution obscures any distinct spiral structure. The galaxy exhibits no obvious signs of major mergers or significant tidal disturbances, although minor irregularities cannot be ruled out due to image resolution. It has a relatively smooth appearance, not exhibiting any features of active galactic nuclei.
