This galaxy appears to be a luminous elliptical galaxy with an overall yellowish hue, indicating an older stellar population with relatively little ongoing star formation. The galaxy's morphology is largely smooth, with no obvious spiral arms or a distinct disk structure. It exhibits a somewhat elongated shape but is mostly rounded. There is evidence suggesting possible minor gravitational interactions, as indicated by faint asymmetries or disturbances in its outer regions. The galaxy is a substantial object and lies at a considerable distance, given its redshift.
