The galaxy presents as a generally smooth, rounded object with a concentrated central region. The color profile indicates a significant presence of older stellar populations. The overall morphology suggests a spheroidal galaxy, likely an elliptical or S0 type. There is minimal evidence of spiral arm structure or dust lanes, further supporting a classification as a galaxy with little active star formation. There is a slight color gradient from the center outwards, which may indicate subtle variations in stellar population or metallicity. The absence of pronounced tidal features suggests it is not undergoing a major merger event, although subtle disturbances might be present upon closer inspection.
