The galaxy presents as a smooth, elliptical structure with a concentrated central bulge that emanates a significant amount of light. It appears to be a galaxy with relatively little active star formation. The galaxy is more elongated than it is round and does not have any obvious signs of a recent major merger or other significant interactions. The light profile appears to be relatively smooth across the galaxy, with a distinct gradient in brightness from the core outwards, with the core being the brightest. There is a notable color gradient where the central bulge is more yellow-red and the color shifts slightly bluer further out. This bluer color could indicate the presence of some younger stars in the outer regions. 
