The galaxy presents as a centrally concentrated object, appearing largely smooth in morphology. The light profile suggests a dominant bulge component, with a gradual decrease in luminosity outwards from the core. The galaxy exhibits a yellowish hue in the central region, transitioning to redder tones in the outskirts, which may indicate an older stellar population. There are no immediately obvious spiral arms or distinct features indicative of ongoing major star formation in the image. The overall structure appears relatively undisturbed, lacking signs of recent or ongoing merger activity. The shape of the galaxy appears more rounded and less elongated.
