The galaxy presents a generally smooth and elliptical appearance. It exhibits a bright central bulge that gradually fades into a surrounding halo. The galaxy displays a yellowish-white hue, suggesting a relatively older stellar population with fewer young, massive stars. There's a subtle elongation, indicating it is more lenticular than perfectly spherical in shape. No distinct spiral arms or features are visible, which further corroborates its classification as an elliptical or lenticular galaxy. Given the estimated redshift, this galaxy is a significant distance away, contributing to the slight blurring of its structural details in the image. The light distribution is centrally concentrated with a fairly even decline away from the core. There's no visual indication of major ongoing mergers, although minor disturbances cannot be entirely ruled out based on the given image quality.
