The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct disk structure. The color profile suggests a dominant population of older stars, exhibiting a yellowish-red hue in the central regions. The outer regions of the galaxy show a gradual decline in surface brightness. The galaxy is mostly round in shape with some ellipticity, but there are no obvious signs of recent major mergers or tidal disturbances in this image. Any star formation is likely subdued within this system, due to a low fraction of blue light. 
