The galaxy presents a primarily elliptical morphology, displaying a smooth, concentrated luminosity profile. Its overall structure is dominated by a centrally concentrated bulge that appears nearly spherical. The color gradient shifts from a yellowish-white core to a subtly bluer halo, suggesting a potential difference in stellar populations; the core likely hosts older, redder stars, while the outer regions may contain younger, bluer stars. There is no clear evidence of spiral arms or a distinct disk. The galaxy exhibits minimal signs of recent merger activity or tidal disturbances, based on the lack of pronounced asymmetries or stellar streams. Given its red color and smooth morphology, it is likely an early-type galaxy. The low-level of star formation, is consistent with a galaxy dominated by older stellar populations.
