The galaxy presents as a flattened, elongated structure, suggesting a likely edge-on spiral or lenticular morphology. The primary light emission appears concentrated along the central axis, indicative of a galactic disk. There is a subtle color gradient visible across the galaxy's body, with a slightly bluer hue at the very edges potentially indicating regions of younger stars or ongoing star formation, although this is hard to confirm given the image resolution. The central bulge is not distinctly prominent, appearing relatively faint and elongated rather than spherical. There are no clear signs of significant dust lanes or prominent spiral arm structures visible in this image. The overall appearance suggests a relatively undisturbed and isolated system.
