The galaxy presents as an elliptical morphology, appearing largely smooth and somewhat rounded in shape. There is evidence of a possible merging event with another galaxy, or at least some form of disturbance in its structure. It displays a color gradient, transitioning from bluer hues on one side to redder tones on the other. This could indicate variations in stellar populations, dust content, or star formation rates across the galaxy. There are no obvious spiral arm structures or a distinct disk component visible in this image.
