The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge, and a fainter halo. The core exhibits a bright, yellowish-white color, suggesting an older stellar population dominating the region. Moving outward from the core, the galaxy exhibits a more diffuse, reddish-yellow hue, indicating a mix of stellar populations, but with a likely presence of dust obscuration. The galaxy appears to have a relatively symmetric profile. The overall structure appears relatively undisturbed, with no clear signs of recent major merger events or tidal disruptions.
