This galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated light profile with a gradual decrease in surface brightness extending outwards. The core region presents a yellowish hue, suggesting an older stellar population. The outer regions show bluer tints, hinting at the presence of some younger, hotter stars, albeit less prominent. There are no easily discernible spiral arms or significant dust lanes visible. The galaxy shows a fairly symmetrical form with a slight deviation toward roundness. The image doesn't show any major signs of mergers or tidal disturbances. The overall color suggests moderate star formation activity.
