The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or significant dust lanes. The color profile suggests a population of older stars, as indicated by the yellow-red hue dominating the central region. There is a slight elongation, but overall it appears largely rounded. Based on its morphology, it may be classified as an elliptical galaxy, with little recent star formation. There are no strong indications of ongoing merger activity or tidal disturbances.
