The galaxy appears to be a relatively smooth, single structure. It exhibits a generally elliptical shape, appearing more elongated than perfectly circular. The primary color is a yellowish-orange, suggestive of an older stellar population. The galaxy's light profile seems concentrated, lacking prominent spiral arms or distinct features typical of younger, disk-dominated galaxies. There is a subtle color gradient visible, with a slightly bluer tinge towards one end of the major axis. This could indicate a small region of localized, recent star formation. While no major disturbances are immediately apparent, there may be a subtle asymmetry in the light distribution, suggesting a possible past minor interaction or merger event. Overall, the galaxy appears to be a massive, relatively evolved system at a moderate redshift.
