The galaxy presents as a predominantly smooth, elliptical-like structure with an oblate shape. The light distribution appears concentrated towards the center, indicating a bright, dense core. The color gradient suggests a population of older stars, with a general yellow-orange hue throughout the galaxy body, though it is not very pronounced. There is a hint of a disk structure, with very faintly visible arms or distortions along the outer edges. These arms do not extend very far and are not sharply defined. There is little evidence of active star formation based on the limited color information available; it appears to be a galaxy transitioning away from forming stars.
