The galaxy appears as a centrally concentrated, yellowish-orange spheroid. Its overall structure suggests a relatively smooth distribution of light. The concentration of light is highest at the core, gradually decreasing outwards, with no apparent spiral arm structures or distinct features indicating recent or ongoing major merger activity. There might be very minor irregular features, but they are not prominent. The object's profile is moderately circular, with a slight deviation towards an elongated shape. The color suggests an older stellar population and reduced star formation activity.
