The galaxy presents as an elliptical morphology, with a smooth, centralized concentration of light. The core region exhibits a yellowish-white hue, indicative of an older stellar population. The light intensity decreases gradually from the center outwards, with a noticeable lack of spiral arm structures or distinct features. The overall structure appears relatively undisturbed. A subtle gradient from the core to the outer regions can be observed, trending towards a slightly redder color. The galaxy's form suggests a well-evolved system, likely having undergone significant morphological evolution. The observed redshift indicates that this galaxy is located at a considerable distance from our own.
