The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. Its overall shape approximates a spheroid, exhibiting high degree of circular symmetry. There is a radial color gradient, with the central region displaying a yellowish-white hue, transitioning to a redder color in the outer regions. No spiral arm structures or prominent dust lanes are discernible. The galaxy appears to be isolated, showing no signs of tidal interactions or ongoing merger activity. The light profile suggests a relatively old stellar population, with minimal evidence of recent star formation within this system.
