The galaxy appears as a flattened, elliptical shape, elongated significantly along one axis. Its color profile suggests an older stellar population, with a prominent yellowish-orange hue dominating the central region. There is a slight gradient in color, with the core appearing more intensely yellow and the outer regions fading to a more diffuse, slightly redder tone. The overall appearance is smooth, lacking distinct features such as spiral arms or prominent dust lanes. Given its shape and color, the galaxy likely has a considerable stellar mass and a relatively low rate of ongoing star formation. There is no apparent sign of any major mergers occurring.
