The galaxy appears as a relatively smooth, centrally concentrated object. The overall shape is elliptical, displaying a moderate degree of roundness. The central region exhibits a somewhat reddish hue, potentially indicating an older stellar population or significant dust obscuration. Moving outward from the center, the galaxy transitions to a more bluish color, suggesting the presence of younger, hotter stars in these regions. There is a faint indication of a disk-like structure, but no prominent spiral arms or bar features are apparent. There are no obvious signs of major ongoing mergers or significant tidal disturbances, although a minor disturbance cannot be ruled out based on the image alone. The galaxy shows evidence of ongoing star formation, though at a relatively modest rate.
