The galaxy presents a flattened, disk-like morphology, viewed at an inclined angle. A prominent central bulge dominates the core region, displaying a bright, concentrated luminosity profile. The disk exhibits a spiral structure, though the arm features appear somewhat flocculent and not sharply defined. Faint dust lanes are discernible within the disk, particularly on the near side relative to our line of sight. The overall color suggests a mix of stellar populations, with a concentration of older, redder stars in the bulge, and hints of bluer star formation regions sparsely scattered throughout the disk. The galaxy appears relatively isolated, lacking any obvious signs of ongoing major merger activity. No significant tidal features or extended halos are immediately apparent in this image.
