The galaxy presents as a centrally concentrated, smooth, and generally featureless elliptical system. The light profile appears relatively uniform, with a gradual decline in intensity from the core outwards. The color index suggests a population of older stars, with a yellow-orange hue indicative of a lack of significant recent star formation. There is no obvious disk structure or spiral arms. The galaxy appears to be quite isolated, with no apparent tidal distortions or nearby companions suggesting any ongoing or recent merger activity. Its morphology appears largely undisturbed, suggesting a relatively quiescent evolutionary history.
