The galaxy presents a somewhat elongated, elliptical morphology. A bright, concentrated core region is evident, indicative of a substantial central bulge. The light distribution appears relatively smooth, with no prominent spiral arms or distinct features readily apparent. The galaxy displays a color gradient, transitioning from a yellow-white hue at the core to a slightly redder color in the outer regions. This may be due to the presence of aging stellar populations in the outskirts. No significant dust lanes or signs of recent major merger events are discernible from the image. Overall, the galaxy appears to be an evolved system.
