The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that appears yellowish-white in color, suggesting an older stellar population. The galaxy lacks distinct spiral arms or other prominent features typically associated with disk galaxies. There is a subtle color gradient from the center outwards, with the outer regions displaying a slightly bluer hue, potentially indicating the presence of some younger stars, albeit less prominent than those found in actively star-forming galaxies. The overall morphology suggests a gravitationally relaxed system. The galaxy seems generally isolated, with no obvious signs of a major ongoing merger, although there might be evidence of a minor disturbance or past interaction based on the slight irregularities.
