The galaxy appears to be an elliptical galaxy. It presents a relatively smooth, featureless morphology, with a high degree of central concentration. The core exhibits a bright, yellowish-white color, indicating a population of older stars. The galaxy displays a slight elongation, with a moderate ellipticity, appearing somewhat rugby ball-shaped. It shows an absence of distinct spiral arms or prominent dust lanes. The color gradient suggests a gradual decrease in stellar population age as we move from the core outwards, transitioning from a more yellow center to a bluish hue in the outer regions. The absence of significant disturbances suggests that it is not undergoing any major merging events. It exhibits only a small amount of ongoing star formation.
