The galaxy presents as a relatively smooth, elliptical or lenticular structure, elongated along one axis. A slight color gradient is perceptible, transitioning from a yellower core region to a bluer hue in the outer regions, potentially indicating subtle variations in stellar population age or dust content. No prominent spiral arms or disk-like features are apparent. The galaxy appears relatively undisturbed, with no significant signs of ongoing major merger events. There is a slight possibility of minor interaction with a nearby object given the light asymmetry in the galaxy. Overall, the galaxy's morphology suggests a relatively evolved system, likely with a moderate rate of ongoing star formation.
