The galaxy presents as a relatively smooth, centrally concentrated object. Its shape is approximately round, though possibly slightly elongated. The central region exhibits a bright, yellowish core, suggesting an older stellar population. Fainter, bluer light extends outwards from the core, possibly indicating some low levels of recent star formation. There are no obvious signs of spiral arms or a strong disk component. The galaxy appears largely undisturbed, with no clear evidence of ongoing or recent major mergers, though there is possibly a slight asymmetry or minor irregularity in its outer regions. The overall color profile suggests a spectral energy distribution that is typical of a massive galaxy at moderate redshift.
