The galaxy appears to be a relatively compact, elliptical system. Its morphology is largely smooth, with a high degree of roundness. There is no clear indication of spiral arms or a distinct disk structure. The galaxy exhibits a concentrated central bulge that fades outward into a diffuse halo. The color profile suggests an older stellar population, given the yellowish-orange hue. There's no strong evidence of recent major mergers or significant tidal disturbances.
