The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated, bright core that graduates outward to a diffuse halo. The color profile suggests a significant population of older stars, indicated by the reddish-yellow hue in the central regions, surrounded by a bluer, more active population. There is a notable absence of prominent spiral arm structures or dust lanes. Based on its apparent structure and color, the galaxy appears to be undergoing a low rate of star formation. Close inspection of the galaxy shows a single, somewhat spherical shape, showing no signs of merging.