The galaxy presents a discernible disk structure, with spiral arm features that appear somewhat tightly wound. The central bulge exhibits a pronounced luminosity, suggesting a high stellar density in that region. A faint bar-like structure appears to traverse the central region, which might indicate the presence of a weak or underdeveloped bar. The disk exhibits a slight inclination relative to our line of sight, allowing us to observe some degree of its spiral structure. There is an indication of dust lanes within the disk.
