The subject galaxy presents as an edge-on or highly inclined disk galaxy. The main disk component exhibits a pronounced dust lane obscuring the central bulge region.

The central region itself shows a yellowish color, indicating the presence of older stellar populations. The disk shows a blueish hue. The halo appears disturbed or asymmetric on one side of the galaxy, potentially suggestive of tidal interactions or a recent merger event. There also appears to be a second structure to the side, perhaps caused by the same event or a smaller satellite galaxy. This structure shows the same blueness as parts of the disk. There are no obvious spiral arm structures visible.
