The galaxy presents as a predominantly smooth, elliptical-like structure. It has a relatively high degree of central concentration with a bright, yellowish core. The light gradually decreases from the center, with no obvious substructure such as spiral arms or a bar visible. The overall color is consistent with an older stellar population. The morphology is generally undisturbed, showing no significant signs of ongoing merger activity or tidal distortions. The galaxy appears to be a well-formed, quiescent system. The red shift data indicates the galaxy is at a considerable distance and is relatively massive. The estimated star formation rate is low, indicating the galaxy is likely populated by older stars.