The galaxy exhibits a flattened, disk-like morphology, presenting itself nearly edge-on to our line of sight. A prominent central bulge is visible, exhibiting a high degree of luminosity and a smooth texture. The bulge is more luminous than the rest of the galaxy. Faint, elongated dust lanes appear partially obscuring the disk. Some asymmetrical features are visible in the disk and potential tidal distortion on one side, indicating signs of an ongoing or recent interaction or merger.
