The galaxy presents as a smooth, elliptical-like structure with a concentrated central bulge that graduates outward to the dimmer edges. The central region exhibits a yellow-orange hue, suggesting an older stellar population and diminished recent star formation. The outer regions are less defined, the color indicates that they are comprised of older, redder stars. There is no clear spiral arm structure evident in the image, and no prominent dust lanes. The overall morphology suggests a lack of significant recent merger activity.
