The galaxy presents as a relatively smooth and featureless elliptical type, with a high degree of central concentration. The light distribution appears largely uniform, lacking prominent spiral arms or distinct substructures. The overall shape approximates an elliptical morphology, being rounded rather than highly elongated or cigar-shaped. The color profile indicates a dominance of older stellar populations, exhibiting a yellowish hue that suggests relatively little ongoing star formation. There is no apparent evidence of significant tidal disturbances or ongoing merger activity, with a smooth light profile.
