The galaxy presents a generally smooth morphology, with a near-circular, relatively undisturbed appearance. Its light profile suggests minimal disk-like structure or spiral arms. The central region appears slightly brighter and more concentrated than the outer regions. There is a slight hint of a perturbation in the galaxy's shape, but no strong indications of a major ongoing merger. The galaxy exhibits a colour gradient, appearing bluer in the centre and more red in the outer regions. This implies that the central region may have younger stars and active star formation, while the outer regions are likely comprised of older stellar populations. Overall, the galaxy appears as a somewhat isolated, relatively evolved system.
