The galaxy appears as a slightly elongated, centrally concentrated object with a smooth, diffuse profile. It presents a largely featureless morphology, lacking prominent spiral arms or a distinct bar structure. The color gradient suggests a redder core, possibly indicating an older stellar population in the center. There's a hint of bluer regions extending outward from the core, which could signify areas of more recent star formation. There is no evidence of any major merger events or tidal disturbances. Overall, the galaxy appears to be an elliptical or lenticular galaxy.
