The galaxy presents as a well-defined, elliptical structure with a smooth overall appearance. It is not perfectly circular, exhibiting a slightly elongated shape. The central region appears to be dominated by older stellar populations, indicated by a reddish hue. Moving outward from the center, the color transitions to a more greenish-blue, suggesting the presence of some younger, hotter stars, perhaps resulting from ongoing or recent star formation, albeit at a moderate level. There is no evidence of significant dust lanes, spiral arms, or other prominent features typically associated with actively star-forming galaxies, nor is there any evidence of a recent major merger. Small scale disturbances cannot be ruled out. The general morphology indicates that this system is relatively evolved.
