The galaxy presents an overall elliptical morphology, appearing as a smooth, centrally concentrated object. The light distribution indicates a relatively uniform and diffuse stellar population, without prominent spiral arm structures or significant dust lanes. The color gradient suggests a population of older stars, resulting in a redder hue throughout the galaxy, particularly in the central regions. There is a moderate degree of ellipticity, with the major axis oriented approximately northeast to southwest. No tidal features or signs of recent major mergers are readily apparent in the immediate vicinity, suggesting that the galaxy has undergone a relatively quiescent evolutionary history.
