This galaxy exhibits characteristics of a spiral galaxy viewed at a slight inclination. A central bulge is apparent, displaying a concentrated, yellowish-white hue indicative of an older stellar population. Surrounding the bulge, the galaxy shows faint spiral arm structures. The arms appear somewhat flocculent and patchy, with hints of bluer regions, likely indicating areas of recent star formation. There is a subtle asymmetry in the arm structure suggesting potential gravitational interaction or past merger event. Dust lanes are subtly observable in the disk structure. Overall, the galaxy's morphology indicates a disk galaxy undergoing active, but possibly declining, star formation. There are no apparent signs of a prominent tidal tail or other significant merger features in this image.
