The galaxy presents as a smooth, elongated structure, likely an elliptical galaxy. The core exhibits a yellowish hue, indicative of an older stellar population. This core gradually diffuses outwards into a surrounding envelope of fainter, bluer light, suggesting the presence of a more dispersed, potentially younger stellar population within the galaxy's outer regions. There are no clear signs of spiral arm structures or dust lanes visible. The overall smooth appearance and the color gradient suggest that the galaxy is relatively undisturbed, showing no major signs of recent mergers or significant star formation. It appears to be a fairly typical example of a galaxy at moderate redshift.
