The object presents as a disk galaxy, viewed at a near edge-on orientation. There is a prominent dust lane visible, bisecting the galaxy along its major axis. This obscuration gives the disk a dark and defined line.

The galaxy exhibits a relatively bright central bulge region which appears to be mostly spheroidal. Color gradients are present throughout the galaxy. The bulge exhibits a yellowish-white hue, suggesting an older stellar population compared to the disk.

The disk shows subtle color variations. Areas appear redder, which could indicate regions of dust and ongoing star formation. Other regions appear bluer which could indicate younger stars.

No obvious signs of a major merger or strong tidal disturbance are apparent in the image, although a slight asymmetry in the outer disk cannot be ruled out. There is a small possibility of a minor disturbance.
