The galaxy presents as a single, relatively smooth object with an elliptical morphology, lacking prominent spiral arms or a distinct disk structure. The central region exhibits a higher surface brightness, appearing yellowish, suggesting an older stellar population. The light seems to gradually fade into the outskirts of the galaxy. There appear to be very faint, diffuse outer regions which are a mix of color, from redder to slightly greener hints, these imply there may be ongoing, albeit minor, star formation. There is no strong evidence of any active galactic nuclei (AGN) based on the image alone. There is no significant morphological distortion visible, indicating a lack of recent major merger events. The overall appearance suggests it might be a relatively massive system, consistent with early-type galaxies at its redshift, with a substantial bulge component.
