The galaxy presents an elliptical morphology, appearing elongated with a cigar-shaped structure. The central region exhibits a high concentration of light, appearing smooth and concentrated, gradually decreasing in intensity towards the outer edges. A subtle color gradient is observed with a yellow-white core transitioning to a bluer halo, indicative of possible differences in stellar populations across the galactic structure. There are no clear signs of spiral arms or significant dust lanes in the visible spectrum. There are no morphological indications of any major recent or ongoing merger activity with another galaxy. The overall appearance suggests a mature galaxy with a dominant spheroidal component.
