The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. Its color is yellowish-white, suggesting a dominant population of older stars. The light distribution appears to be fairly uniform, lacking prominent spiral arms or distinct features. There is minimal evidence of ongoing star formation within the galaxy. The galaxy has an apparent axis ratio near unity, indicating it is close to face-on orientation. Overall, this galaxy is likely a relatively massive, passively evolving system at a redshift of approximately 0.11.
