The galaxy presents as a somewhat elongated, elliptical shape with a smooth, diffuse light distribution. The central region appears brighter and more concentrated, with a gradual fading towards the outer edges. The color profile suggests an older stellar population, evidenced by the yellowish-red hue, indicative of lower star formation activity. There is no clear evidence of spiral arms, dust lanes, or other distinct features. The overall morphology suggests it could be a lenticular galaxy, or an elliptical galaxy seen at an angle.
