The galaxy presents a predominantly elliptical morphology, appearing smooth and relatively featureless. Its shape is somewhere between round and slightly elongated. There is a concentration of light toward the galaxy's core, suggesting a prominent bulge. The galaxy exhibits a color gradient, with a yellowish-white central region and a bluer outer halo, potentially indicating a mix of older stellar populations in the core and younger stars in the surrounding regions. No obvious spiral arms or strong dust lanes are visible. The galaxy appears relatively isolated, with no clear signs of ongoing major merger activity.
