The galaxy presents as a relatively compact and smooth object. Its morphology appears elliptical or perhaps a lenticular type galaxy due to the lack of discernible spiral arm structure or significant dust lanes. The light profile suggests a centrally concentrated brightness, fading gradually outward. Coloration is mostly homogenous with a slight bluer tinge apparent, indicating some ongoing star formation, although overall the stellar population appears relatively old and evolved. There are no signs of tidal features, major disturbances, or ongoing mergers in the immediate vicinity, suggesting a quiescent state. The galaxy exhibits a well-defined, rounded appearance, lacking significant elongation or distortion.
