The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a notable lack of distinct features such as spiral arms or prominent dust lanes. The light profile suggests a relatively even distribution of stars, with the brightest region concentrated in the core. The color gradient indicates a redder hue in the central region, possibly suggesting an older stellar population dominating the core. Fainter, bluer emissions can be seen towards the edge of the object. There is no sign of interaction or a major merger event. 
