The galaxy appears to be a spiral galaxy, seen at an inclined angle relative to our line of sight. The disk component is evident, though not perfectly edge-on. Two dominant spiral arms are visible, tracing out from the central bulge region. These arms display a loose winding pattern. The central bulge exhibits a moderate size in comparison to the overall galaxy. There are no obvious signs of significant tidal disturbances or major mergers. The bulge region appears relatively smooth in texture, while the spiral arms show hints of clumpy structure, potentially indicative of star formation regions. There is a weak presence of a bar feature that goes through the central bulge. 
