The galaxy presents as a generally smooth, centrally concentrated structure with a bright, yellowish core that graduates to a dimmer, greenish halo. It exhibits a somewhat elliptical morphology, appearing more rounded than elongated. There is no prominent disk structure or spiral arm features readily visible. Indications of any ongoing or recent merger activity are not apparent, as the galaxy appears to be a fairly isolated and relatively undisturbed system. It is likely an elliptical galaxy, with low star formation.
