The galaxy presents a clear edge-on disk morphology. There is a prominent central bulge, appearing to be somewhat rounded in shape. Little to no spiral arm structure is discernible. The disk appears relatively smooth with no major dust lanes or knots visible. The color gradient suggests the presence of both older stellar populations (redder hues) and younger, star-forming regions (bluer hues), albeit subdued. The galaxy exhibits a relatively high degree of symmetry around its major axis. The overall luminosity indicates a massive galaxy. Based on this, it is likely a spiral galaxy.
