The galaxy presents as a relatively compact and luminous object. Its overall morphology appears smooth, lacking prominent spiral arms or a well-defined disk structure. There is a slight color gradient from the center outwards. Its shape is somewhere between round and elliptical. There is no obvious sign of a major merger event, though minor disturbances cannot be ruled out from this image alone. Based on its apparent color, the galaxy is likely an older stellar population and lower levels of star formation.
