The galaxy appears as a centrally concentrated elliptical system. The core exhibits a bright, yellowish hue, indicative of an older stellar population. Moving outward from the core, the galaxy gradually fades into a fainter, more diffuse halo. There is a subtle elongation to the galaxy's overall shape, deviating slightly from a perfect circle. No distinct spiral arm structures or significant dust lanes are apparent within the visible light spectrum. There is no indication of major disturbances or ongoing merging events. The smooth light profile suggests a relatively quiescent galaxy. The overall color gradient from the core to the outer regions is subtle, with the yellowish core transitioning to slightly redder tones in the outer halo, suggesting potential differences in stellar populations or metallicity.
