The galaxy presents a generally smooth, elliptical morphology. Its light profile suggests a high degree of central concentration. There's a noticeable color gradient, shifting from a bluer hue in the outer regions to a redder, yellower core, which could indicate an older stellar population dominating the central bulge. The disk is at an angle, it could be a spiral galaxy. The galaxy appears undisturbed, with no obvious signs of recent mergers or major tidal interactions.
