The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a slightly elongated, elliptical shape with a hint of asymmetry. The core appears bright and diffuse, emitting primarily in the blue-green wavelengths, which fades into a dimmer, redder halo. There is evidence of minor disturbances in the morphology, possibly indicating an interaction or past merger event. The overall structure suggests an evolved system, potentially an elliptical galaxy with ongoing, but relatively low, star formation.
