The galaxy appears as a single, centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish hue, possibly indicating an older stellar population. There is a subtle radial gradient in color, with the outer regions appearing slightly redder and less luminous, which could be due to a change in stellar population or dust content. The overall form is quite regular, without any obvious signs of spiral arms, bars, or major disturbances. There are no pronounced tidal tails or close companion galaxies visible in the immediate vicinity, suggesting it is not currently undergoing a major merger event.
