The object appears to be a relatively smooth galaxy with a concentrated central bulge. It exhibits a somewhat elliptical morphology, appearing to be largely spheroidal in shape rather than disk-dominated. The color gradient suggests a population of older stars, with the core appearing yellow-white and the outer regions taking on a slightly redder hue. There is little evidence of spiral arms or significant dust lanes, further supporting the classification as an elliptical or S0 galaxy. The smooth appearance indicates minimal recent merger activity or star formation. The faintness of the outer regions of the galaxy indicates a gradual decline in stellar density. It shows only minor disturbances.