The galaxy presents an overall elliptical morphology, exhibiting a smooth, diffuse light distribution rather than well-defined spiral arms or a prominent disk structure. Its color appears generally redder, indicative of an older stellar population with suppressed ongoing star formation. There is evidence of a potential merger event occurring, possibly with another galaxy. The main body of the galaxy exhibits a somewhat disturbed structure. It is likely a massive galaxy, given its luminosity at its redshift. The half-light radius is approximately 11 kiloparsecs. There is a central concentration of light.