The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. Its core exhibits a bright, yellowish-orange hue, suggesting an older stellar population dominating this region. The light appears to gradually diffuse outwards from the core, transitioning to a fainter, redder shade along the galaxy's outer edges. There is a slight elongation, but it appears mostly round. There are no visually discernible spiral arms, dust lanes, or other distinct features indicative of active star formation or recent merger activity.
