The galaxy presents as an elliptical morphology with a moderate axis ratio, appearing somewhat elongated but not highly flattened. It exhibits a smooth, diffuse profile lacking distinct spiral arm structures or prominent dust lanes. The central region appears brighter, indicative of a concentration of stars, possibly a galactic bulge. The color gradient suggests a relatively evolved stellar population, transitioning from bluer hues in the outer regions to a more uniform color in the inner regions. A potential tidal tail is noted, hinting at a possible past interaction or merger event. The overall appearance of the galaxy implies a dynamically relaxed system with ongoing, albeit subdued, star formation.
