The galaxy presents as a somewhat elliptical structure with a smooth, diffuse morphology. The core region exhibits a bright, concentrated luminosity, suggesting a high stellar density. A subtle color gradient is observable, transitioning from a yellowish-white hue in the center to a slightly bluer periphery. The outer regions fade gradually into the background sky, indicating a lack of distinct, well-defined spiral arms or prominent features. A possible faint disk component may be present but is not sharply defined. Overall, the galaxy appears relatively undisturbed, without major signs of tidal interactions or recent merger events.
