The galaxy presents as an elongated structure, consistent with a disk galaxy viewed nearly edge-on. There is a central bulge which appears relatively smooth and concentrated. The disk component exhibits a slight warp and is visibly thinner, displaying a dusty appearance in its darker shades. Some faint, diffuse features extend from the main body of the galaxy. The color gradient suggests an older stellar population. The color is predominantly orange, with less blue, indicating a lower rate of ongoing star formation. Any evidence of spiral arms is obscured by the edge-on view. No obvious signs of recent major merger events are evident in this image, but slight asymmetries in the disk could indicate minor interactions.
