The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. It exhibits a round morphology with a subtle color gradient, transitioning from a more yellow-green hue in the central region to a redder tint at the edges. This suggests a possible older stellar population in the galaxy's core with some indication of potential ongoing star formation. There is no visible spiral structure or significant dust lane obscuration. The galaxy appears mostly undisturbed, with no obvious signs of major mergers or tidal interactions, although a minor disturbance cannot be ruled out. Based on the color profile, it is likely a massive galaxy with a moderate rate of star formation.
