The galaxy appears to be a spiral galaxy, observed at a near edge-on orientation. There is a prominent central bulge that appears to be a moderate size compared to the full galaxy. A potential bar structure is seen in the center as well. Spiral arms are visible as they extend from the bulge, showcasing moderate winding, appearing well-defined. The image reveals a blue disk of stars that spreads outwards, appearing flat, with likely a larger redder bulge. The galaxy's disk structure suggests it has not undergone any significant merger events in its recent past, but instead is a mature, isolated galaxy. There are no signs of strong tidal distortions.