The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. The core is bright and appears yellowish-white, suggesting an older stellar population. Moving outward from the core, the color transitions to a more reddish hue. The shape of the galaxy is elongated, with the major axis oriented at approximately 125 degrees. The galaxy is not perfectly elliptical; there are subtle irregularities in its outline, but it does not show signs of major disturbances. The outskirts fade gradually into the background sky, implying a well-defined edge to the galaxy's visible stellar distribution. There does not appear to be any prominent dust lane or spiral arm structure. Overall, it seems to be a large, relatively massive galaxy with a substantial population of older stars.
