The galaxy presents as a relatively smooth and centrally concentrated structure. It exhibits an overall elliptical morphology, appearing elongated rather than perfectly spherical. The central region displays a yellowish hue, likely indicating an older stellar population. Moving outward from the center, the color transitions to a bluer shade, possibly due to the presence of younger, hotter stars. These bluer regions appear to be somewhat patchy and unevenly distributed throughout the galaxy's outskirts. No prominent spiral arms or distinct dust lanes are visible. The galaxy does not appear to be strongly interacting with any other object, though there are faint, disturbed features surrounding the core. Based on its redshift, we are looking at this galaxy as it was a significant time ago.
