The galaxy presents a smooth, elliptical morphology. A concentrated, bright core transitions outward to a more diffuse halo. The galaxy exhibits a color gradient, appearing more yellow-orange toward the center, suggesting a higher concentration of older stellar populations. Fainter bluish regions are subtly apparent in the outer areas. These areas may indicate localized pockets of younger, hotter stars forming within the galaxy's outskirts. There is no strong indication of a prominent disk structure or spiral arms. The general symmetry and lack of significant disturbances suggest the galaxy is relatively relaxed, with no ongoing major merger activity easily discernible in this image.
