The galaxy presents as a smooth, elliptical form with a concentrated central bulge that is bright yellow-orange. Moving outward from the core, the luminosity decreases gradually, and the color shifts toward a redder hue. No distinct spiral arm structures or dust lanes are discernible. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal disruptions. It exhibits a slight elongation, leaning towards a cigar shape, rather than a perfectly circular appearance. Based on its color and morphology, this galaxy is likely comprised predominantly of older stellar populations with minimal ongoing star formation.
