This galaxy presents a relatively smooth, elliptical morphology. It displays a moderate color gradient, transitioning from a slightly bluer hue at the center to redder tones in the outer regions, suggestive of a potential centrally concentrated stellar population with ongoing, albeit low, star formation. There is some evidence of minor disturbances in the galaxy's form, perhaps indicative of tidal interactions or a recent minor merger event. Overall, the galaxy appears to be relatively undisturbed and well-defined.
