The galaxy appears as a centrally concentrated object with a relatively smooth, featureless morphology. The light profile suggests an elliptical or lenticular galaxy, with a bright nucleus that decreases in intensity toward its outer regions. It appears nearly face-on but with some evidence of oblateness. It exhibits a yellowish-white color, suggestive of an older stellar population with relatively low current star formation, though some blue light may be present. It is neither a late-type spiral galaxy nor an actively merging system. The smooth appearance indicates that it has likely undergone a period of quiescence, or is in a state of slow, steady evolution. The morphology seems relatively undisturbed with the exception of a few minor features. There appear to be no distinct spiral arms or prominent dust lanes visible in this image.
