The galaxy presents as a largely featureless, elliptical morphology with high degree of central concentration. The galaxy core exhibits a bright, yellowish-white hue which gradually diffuses outward into a more reddish-yellow extended halo. There is no readily apparent structure such as spiral arms, dust lanes, or prominent star-forming regions. The overall appearance suggests a relatively smooth distribution of stellar populations, characteristic of evolved stellar systems, potentially with a low ongoing star formation rate. There is no evidence of any major ongoing merger activity. Minor distortions are not resolvable at this level. The overall form is highly circular.
