The galaxy presents as a single, centrally concentrated object with a generally smooth appearance. The light profile suggests a spheroidal morphology, potentially an elliptical galaxy or the bulge component of a spiral galaxy observed at a distance where finer details are not readily discernible. The core region is relatively bright with a yellow hue, possibly indicating an older stellar population. This yellow light fades into a more pale green colored halo. The overall color profile indicates a moderate degree of stellar formation activity. There's no readily apparent signs of ongoing merger activity or significant tidal disturbances in the image.
