The galaxy presents as a moderately bright, relatively compact object. Its morphology is predominantly smooth, with a high degree of central concentration. The light distribution appears approximately elliptical. There is a color gradient, with the core exhibiting a more yellow-orange hue, suggesting an older stellar population and/or dust obscuration. The outer regions display a bluer tint, potentially indicative of younger stars, although this is subtle. There is no obvious spiral structure or prominent dust lanes visible. There is no indication of any recent or ongoing major merger events. Minor asymmetries or distortions are not apparent. The galaxy is likely an early-type galaxy, potentially an elliptical or S0. The redshift suggests it is at a considerable distance.
