The galaxy appears as an elliptical structure, with a relatively smooth and featureless morphology. It exhibits a moderate degree of ellipticity, appearing more "in between" round and cigar shaped. There is no visual evidence of a prominent disk component. Color gradients suggest a more luminous core region compared to its outer regions. There is no obvious visual evidence of any major ongoing merger or strong tidal disturbance, though minor disturbances cannot be fully ruled out based on visual inspection alone. The overall light distribution is relatively concentrated. The galaxy appears to have undergone minimal morphological disturbance.