The galaxy presents a relatively smooth, elliptical morphology with a high degree of central concentration. The light profile suggests a spheroidal shape, appearing mostly round, with only a slight deviation towards an intermediate form. There is evidence of a possible minor interaction or disturbance in the form of a second condensation of light near to the main body. This could indicate a galaxy merger. The galaxy exhibits colors consistent with moderate star formation activity, with some regions displaying bluer tints indicative of younger stellar populations. 
