The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that gradually diffuses outwards. There are subtle color variations, with the central region appearing more yellow or golden, possibly indicating an older stellar population. There are no distinct spiral arms or prominent dust lanes visible, which suggests a lack of significant ongoing star formation within a clearly defined disk. There are no apparent signs of recent major merger activity or significant tidal disturbances in its immediate morphology. The overall shape indicates a galaxy that is likely close to spheroidal.
