The galaxy presents as an elliptical morphology with a smooth, centrally concentrated light profile. The core region exhibits a bright, yellowish hue indicative of an older stellar population. The galaxy displays a moderate degree of ellipticity, appearing slightly elongated rather than perfectly spherical. There is no readily apparent disk structure or spiral arm features. Evidence of recent or ongoing major merging events are absent; however, there might be minor disturbances observable. The outer regions fade gradually into the background sky, lacking any sharp truncation in surface brightness. Overall, the galaxy appears as a relatively undisturbed elliptical galaxy at a moderate redshift.
