The galaxy appears to be a relatively smooth object, likely an elliptical or lenticular type, with a dominant central bulge and a lack of well-defined spiral arms or disk structure. Its overall shape is generally round. There is a slight elongation. The galaxy's color is dominated by what appears to be light in the green part of the spectrum, suggesting a stellar population that is not very dusty. The central region of the galaxy seems to be brighter than the outer regions, as expected. There is no obvious visual evidence of any major ongoing merger events or strong tidal disturbances. A faint, diffuse halo or envelope might be present but is not clearly resolved.
