The galaxy presents as a primarily smooth, elliptical form. The central region exhibits a concentrated luminosity, suggesting a significant stellar density and potentially an active galactic nucleus, though further spectral analysis would be needed to confirm this. The radial color gradient displays a shift from a yellow-white core to a redder halo, possibly indicating older stellar populations in the outer regions. The galaxy displays a notable lack of discernible spiral arm structures or dust lanes. There is only a very minor disturbance observable. It presents as a somewhat large galaxy.
