The galaxy appears as a centrally concentrated object with a largely smooth morphology. Its shape is somewhat elliptical, displaying a slight elongation. The primary light emission originates from a yellowish-orange core region, suggesting an older stellar population. Fainter, bluish-green extended emission surrounds the core, potentially indicative of more recent, albeit low, star formation activity. There are no prominent spiral arm structures or significant signs of ongoing merger events visible in this image. The overall structure points toward a galaxy possibly transitioning toward an elliptical morphology with diminished star formation.
