The galaxy exhibits a generally smooth, elliptical morphology with a concentrated central bulge. The color profile suggests a redder core transitioning to a slightly bluer halo, indicative of an older stellar population dominating the central region with potentially younger stars at the periphery. There is a subtle asymmetry, possibly suggesting a minor gravitational interaction or an internal disk-like structure viewed at an angle. No prominent spiral arms or bar features are discernible within the resolution limits of the image. The overall structure is relatively undisturbed, with no obvious signs of a major ongoing merger event.
