The galaxy presents as a spiral type, observed at a redshift that indicates a considerable distance. It exhibits a prominent central bulge, which appears relatively smooth and concentrated, suggesting a significant population of older stars. The overall color profile indicates a strong presence of yellow, which is likely indicative of an older stellar population. The spiral arms, while present, appear somewhat flocculent and less well-defined, with a moderate degree of winding. There is evidence of ongoing star formation within the disk, particularly along the spiral arms, marked by some areas of bluer light that are dispersed throughout. A faint bar structure is discernible, oriented across the central region of the galaxy. The disk component displays an inclination that allows for a partial view of the spiral structure. No significant signs of a major ongoing merger or strong tidal disturbances are observed, though subtle asymmetries may suggest minor gravitational interactions.
