The galaxy presents as a centrally concentrated object, with a smooth, elliptical morphology. The core exhibits a bright, yellowish hue, suggesting a population of older stars. Fainter reddish and greenish arms extend outwards. The system shows a hint of disturbance on one side, potentially suggestive of minor tidal interactions or a minor merger event. The overall structure indicates a relatively evolved system, with ongoing, but potentially low, star formation. The outer regions are fainter and less defined, hinting at a gradual transition to the intergalactic medium.
