The galaxy presents as a centrally concentrated, relatively smooth structure. It exhibits a flattened spheroidal shape, appearing more rounded than elongated. There's no obvious spiral arm structure visible, and the color profile suggests a relatively homogeneous stellar population across the galaxy. The central region appears brighter and slightly redder, indicative of an older stellar population or dust concentration. Subtle irregularities are present in the outer regions, though these do not strongly suggest any major ongoing merger activity. There are hints of a faint disk but it seems to be mostly spheroidal in structure. Overall, the galaxy appears to be a relatively undisturbed system.
