The galaxy presents a generally smooth morphology, appearing as an elongated spheroid. The central region exhibits a high concentration of light, which gradually diminishes towards the outer edges. The color profile suggests an evolved stellar population, leaning towards redder hues in the core. Evidence of a disk is not immediately apparent, hinting toward classification as an elliptical galaxy. There is no visual indication of significant ongoing star formation, nor does there appear to be a major ongoing merger event. Subtle irregularities may exist in the outer halo but overall the system seems relatively undisturbed. The galaxy appears to be fairly massive, as hinted by its considerable luminosity.
