The galaxy presents as a lenticular-like structure with a smooth, centrally concentrated bulge. The overall color of the galaxy is a yellow/orange hue, indicating an older stellar population with minimal ongoing star formation. There is a hint of a disk component, though it appears relatively featureless and without prominent spiral arms. The morphology suggests a system that has largely exhausted its gas supply, resulting in a diminished star formation rate and a population dominated by older, redder stars. There is some evidence of a minor gravitational disturbance from a possible past interaction or merger, but the overall structure remains relatively undisturbed.
