The galaxy presents a flattened, elongated morphology, indicative of a disk-like structure viewed at an oblique angle. The central region exhibits a concentrated luminosity, suggesting the presence of a bulge. Color gradients are noticeable, with a tendency towards redder hues in the central bulge region and potentially bluer tones in the outer disk. The overall color profile suggests a mature stellar population, particularly in the bulge. There is little to no visible evidence of active star formation regions, such as prominent HII regions or spiral arm structures. The galaxy appears relatively undisturbed, with no clear signs of major mergers or tidal distortions.
