The object appears to be a single, relatively smooth galaxy. It appears mostly elliptical and only slightly elongated in shape. There is no obvious central bulge or spiral arm structure visible. The color profile appears relatively uniform across the galaxy, suggesting a lack of significant dust lanes or areas of intense star formation. The galaxy exhibits a color gradient, appearing bluer in the center and becoming redder towards its periphery. This suggests a possible variation in stellar populations, with younger, hotter stars concentrated in the core. No clear signs of tidal disturbances or ongoing major merger events are immediately apparent, although the presence of a minor disturbance cannot be entirely ruled out. 
