The galaxy presents as a disk galaxy observed nearly edge-on. A prominent dust lane obscures the central region, bisecting the galaxy's light profile and indicating the presence of a significant gas and dust component within the disk. The galaxy appears to be relatively smooth, with no obvious signs of strong spiral arm structure or significant star-forming regions beyond the inner disk. The bulge is visible, but is not particularly prominent relative to the disk. The overall morphology suggests a relatively mature galaxy. There are no visible signs of recent major merger activity or significant tidal distortions, though some minor irregularities cannot be ruled out. The galaxy displays a color gradient, with the central bulge appearing yellower than the outer disk.