The galaxy presents as a singular, somewhat concentrated luminous object. Its overall morphology appears relatively smooth, exhibiting a general elliptical form without prominent spiral arms or significant structural irregularities visible in this image. The color is primarily red-shifted, skewing towards yellow-orange hues, suggesting an older stellar population and/or dust obscuration. There is no immediately obvious indication of ongoing major star formation or merging events. Overall, the galaxy appears to be relatively quiescent and evolved.
