This galaxy presents as a flattened, disk-like structure with a distinct central bulge. The bulge appears relatively concentrated, exhibiting a bright, nearly uniform luminosity. The disk component is oriented approximately edge-on to our line of sight, obscuring detailed spiral arm structure if any exists. There is a subtle indication of warping or possible tidal disturbances along the outer edges of the disk. The galaxy's color appears relatively uniform, displaying a pale blue hue with a hint of green in the outer edge, suggesting the presence of younger, hotter stellar populations. However, the overall color does not strongly indicate a dominant population of either young, star-forming regions or older, redder stars.
