The galaxy presents an elliptical morphology. Its overall light distribution is smooth and concentrated toward the center, indicating a relatively old stellar population with minimal ongoing star formation. The color gradient suggests a redder core, possibly due to older, cooler stars and a slight presence of dust. There is a subtle disk-like feature present in the galaxy's structure, with a weak blue hue that might indicate the presence of a young population of stars. Overall, the galaxy appears isolated, with no obvious signs of interaction or merging activity.
