The galaxy exhibits a smooth, elliptical morphology, appearing largely featureless. Its overall shape is roughly intermediate between perfectly round and elongated. There are no readily apparent spiral arms or bar structures. The galaxy's color gradient shows a tendency toward redder hues, potentially indicative of an older stellar population or a higher concentration of dust. There is no indication of any ongoing major merger activity. The image does not clearly rule out minor disturbances. Based on these observations, the galaxy likely represents an evolved system with reduced star formation.
