The galaxy presents a flattened, elliptical morphology when observed from our vantage point. The light distribution is concentrated towards the center, with a smooth and diffused appearance, decreasing in intensity towards the outer edges. There is an indication of a disk-like structure, viewed at a shallow angle. A subtle color gradient is observed, transitioning from a yellow-tinged core to somewhat bluer outer regions. Overall, this appears to be a relatively undisturbed galaxy, exhibiting characteristics indicative of aging stellar populations and minimal ongoing star formation.
