This galaxy presents a seemingly spheroidal morphology, appearing relatively smooth in structure. It exhibits a yellowish-orange hue, indicative of an older stellar population. There appears to be a dual-lobed central structure, possibly suggesting an ongoing or recent merger event. There is a slight asymmetry in the overall shape, with hints of tidal disturbances, further supporting the possibility of interaction with another galaxy or past merger activity. The overall color profile suggests minimal ongoing star formation.
