The galaxy presents a smooth, elliptical morphology, with a high degree of central concentration. Its shape is nearly circular but shows some degree of elongation. The light distribution decreases smoothly from the center outwards. The galaxy has a prominent bulge and little evidence of a disk structure or spiral arms. There is no evidence of ongoing major merger activity or significant tidal disturbances. The galaxy exhibits a color gradient, appearing bluer in its outer regions and redder towards the core. The galaxy is a relatively massive system, characterized by low star formation.