The galaxy presents a largely smooth, elliptical morphology. Its overall color profile indicates a significant population of older stars, which is supported by its elliptical shape. The central bulge is well-defined and exhibits a brighter, yellower hue, suggesting a higher concentration of evolved stars and possibly a supermassive black hole. The galaxy lacks prominent spiral arms or significant dust lanes. There are hints of some disk features within the galaxy. There is no indication of a recent major merger. The galaxy is relatively compact.
