The galaxy appears to be a relatively smooth, elliptical system. The light distribution is centrally concentrated, exhibiting a strong central bulge. There is a subtle gradient in color from the center outwards, with the core appearing more yellow in hue and the outer regions exhibiting a slightly redder tone. No distinct spiral arms or dust lanes are visible. The galaxy's overall shape is slightly elongated, deviating marginally from a perfect sphere but not appearing strongly barred or disc-like. There is no evidence of major tidal disturbances or ongoing merger activity. The light profile suggests that the galaxy is primarily composed of older stellar populations with relatively low levels of current star formation.
