The galaxy presents a largely elliptical morphology, exhibiting a smooth and centrally concentrated light distribution. The color profile suggests a dominant population of older stars, with a yellowish-red hue permeating the galaxy's body. There is little evidence of spiral arms or significant dust lanes, supporting its classification as an elliptical galaxy. The galaxy's shape is generally in-between round and elongated. There is no visual evidence of a recent or ongoing major merger event, though the data suggest that there is possibly minor disturbances. The galaxy's relatively high redshift and absolute magnitude indicate that it is a luminous and massive object.
