The observed galaxy presents a clear disk morphology, viewed almost perfectly edge-on. A central bulge is present, appearing moderately bright with a slightly elongated, roughly rounded shape. Little to no structure is discernible within the disk itself, likely due to the edge-on orientation which obscures spiral arms or dust lanes if they exist. The light from the galaxy appears reddened. The overall appearance suggests a galaxy with relatively low ongoing star formation and a large stellar mass. No signs of major mergers or significant tidal disturbances are apparent in the image, indicating a relatively undisturbed evolutionary history.
