The galaxy presents as a fairly smooth, elliptical-like structure with a concentrated central bulge. The color profile suggests a dominance of older stellar populations, exhibiting a yellowish-orange hue centrally that fades into redder tones towards the outskirts. There's no discernible spiral arm structure or significant dust lane obscuration evident in this image. Overall, the galaxy appears relatively undisturbed, without any obvious signs of recent major mergers or tidal interactions. It is neither perfectly round, nor completely elongated. The galaxy could potentially be undergoing minor disturbances as there are a couple of areas within the galaxy that seem slightly off-center.
