The galaxy presents as a fairly smooth, centrally concentrated object, likely an elliptical galaxy at a moderate redshift. Its overall shape is close to round, exhibiting minimal deviation from circular symmetry. There is no obvious indication of strong spiral arm structure or a prominent galactic disk. Minor disturbances cannot be ruled out, but based on the imaging data, there does not appear to be a major ongoing merger event. The galaxy exhibits a yellow-orange hue, suggesting an older stellar population and low rate of star formation.
