The galaxy appears as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that diminishes gradually into an outer halo. The core appears to have a yellowish-orange color, which may indicate an older stellar population. There is a slight color gradient that transitions to a more greenish hue at the edges, hinting at the presence of some younger stars or ongoing star formation in these outer regions. Overall, the galaxy does not appear to be heavily disturbed, showing no visible signs of recent major mergers or strong tidal interactions with other galaxies. The morphology suggests a galaxy at moderate redshift with a relatively high stellar mass.
