The galaxy appears to be a spiral galaxy, observed at an intermediate redshift. It possesses a notable disk structure, oriented close to face-on. Spiral arms are visible, although somewhat diffuse. The central bulge is of moderate size, neither overly dominant nor negligible. There is a suggestion of a bar structure within the central region. The overall color suggests active star formation, with a hint of recent or ongoing interactions or disturbances within the galaxy, potentially a minor or major merger. The galaxy does not appear entirely smooth; it has both a smooth fraction as well as featured fractions. It is estimated to be a galaxy of considerable mass.
