The galaxy presents a largely smooth, elliptical morphology. Its core exhibits a high degree of central concentration, characterized by a bright, yellow-white hue, indicative of an older stellar population. The galaxy appears somewhat rounded and generally undisturbed with a smooth texture. There is minimal evidence of spiral arm structures or dust lanes within the visible portion of the image. A faint blueish region is seen on the edge of the galaxy, but it is not possible to determine if this is a result of tidal interactions. The overall color gradients suggest a declining rate of star formation, transitioning from a relatively quiescent central region toward slightly more active regions in its outer halo.
