The galaxy presents as a relatively faint, elongated structure with a high degree of inclination with respect to our line of sight. The central region exhibits a concentrated, brighter luminosity suggestive of a bulge or nuclear component. The disk component appears smooth and shows a flattening. The disk's light gradually fades from the galactic center outwards, indicating a decreasing stellar density. Color gradients are subtle, with a slightly bluer hue apparent in the outer disk compared to the yellower central bulge. The overall morphology appears undisturbed, lacking any obvious signs of recent major mergers or tidal interactions.
