The galaxy appears as a singular, moderately concentrated object. It is substantially smooth in overall texture with a high degree of central concentration. There is a moderate gradient in color, transitioning from a yellow-white center to a red-shifted periphery. This color suggests a degree of aging in the stellar populations located within this galaxy. There is no apparent spiral structure or disk component. The light profile suggests a near-spherical, potentially elliptical morphology. There is no observable evidence of recent or ongoing major merger activity. The lack of blue coloration in conjunction with the general smoothness could indicate that it is a relatively quiescent galaxy in terms of current star formation. The object is relatively isolated; only minor disturbances, if any, can be seen around it.