This galaxy exhibits a flattened, disk-like morphology, with a significant degree of inclination relative to our line of sight. The central region presents a bright, yellowish-white core, suggesting an older stellar population and potentially a supermassive black hole. Moving outwards from the core, the disk shows a gradual fading in luminosity. The galaxy exhibits faint spiral arm structures, though they are not sharply defined. They display a bluer hue, indicating ongoing star formation. Hints of dust lanes are present along the disk, particularly on one side, which suggests a degree of asymmetry. Overall the galaxy appears relatively undisturbed, displaying no major signs of recent or ongoing mergers.
