The galaxy presents as a relatively compact object with a smooth, elliptical morphology. There is a lack of any discernible spiral arm structure or a prominent central bulge. The light distribution appears quite uniform, indicating a well-mixed stellar population. A slight elongation is visible, which suggests some level of ellipticity. No significant dust lanes or patches of intense star formation regions are observed. Based on the object's color, it is likely composed of older stellar populations. There may be some evidence of minor disturbances or interactions occurring.
