The galaxy presents as a relatively smooth, centrally concentrated object with a largely elliptical morphology. The light profile appears to decline smoothly from the center outward, exhibiting no discernible spiral arm structure or prominent dust lanes within this image resolution. The core is of brighter luminance and shifts to a yellow coloration, with the outer regions fading to a more diffuse reddish hue, indicating an older stellar population and minimal ongoing star formation. Based on the even color distribution and morphological properties it most likely hosts a smaller number of younger, bluer stars, and its rate of star formation is low. There are no evident signs of major disturbances or tidal features suggesting a recent major merger event. The shape is very close to circular.
