The galaxy presents as a centrally concentrated object with a relatively smooth overall morphology. It appears elliptical in shape, exhibiting a gradual decrease in luminosity from the core outwards. The core region is luminous, indicating a high stellar density or possible AGN activity. The color gradient suggests a redder population of stars dominating, possibly indicating an older stellar population. There is no obvious spiral structure or prominent dust lanes, supporting a classification toward an early-type galaxy. No strong tidal features or obvious signs of recent major merger events are apparent. Subtle disturbances cannot be ruled out given the resolution.
