The galaxy presents as a centrally concentrated, smooth object with a relatively high degree of circularity. The light profile appears to be dominated by an elliptical spheroid, exhibiting a radial gradient in color, shifting from a redder core to a slightly bluer, less concentrated outer halo. This color gradient suggests an older stellar population concentrated towards the center, with a younger stellar population distributed throughout the galaxy. There is little to no evidence of spiral arm structure or a prominent disk. The overall morphology suggests a galaxy in a relatively quiescent state, lacking significant ongoing star formation. There is no visual evidence of tidal disturbances or ongoing merger activity.
