The galaxy presents as a somewhat smooth, elliptical structure with a high degree of central concentration. There is a slight elongation in its overall shape, appearing more cigar-shaped than perfectly round. The galaxy exhibits a color gradient, with the central region appearing a yellow-gold hue, possibly indicating a population of older stars and a relative lack of ongoing star formation. The outer regions show subtle color variations, though the resolution limits definitive identification of distinct features. There's no obvious evidence of major mergers or significant disturbances in its morphology. The galaxy appears generally isolated.
