The galaxy appears to be a relatively smooth, elliptical system. Its morphology is largely spheroidal, with a high degree of central concentration. The light profile indicates a substantial bulge component. There is little evidence of spiral arm structure. The color is predominantly red-yellow, suggestive of an older stellar population with low ongoing star formation. The object exhibits a high degree of circularity; there is no obvious elongation or flattening. No tidal features or signs of recent major merger events are visible. The galaxy may be undergoing minor interactions, though this is not immediately apparent.