The galaxy presents as a singular, largely featureless object. It exhibits an elliptical morphology, appearing elongated with a high degree of central concentration. The light distribution is smooth and diffuse, lacking any discernible spiral arm structures or dust lanes. There is a subtle color gradient visible, with the core region appearing slightly more yellow/gold than the outer regions. The overall color suggests a relatively old stellar population with a low ongoing star formation rate. There is no evidence of any significant merger activity or tidal disturbances affecting its structure. The object appears relatively isolated, without close companion galaxies likely influencing its evolution. 
