The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that dominates the overall light profile. The galaxy appears to be somewhat elongated, with a ratio of major to minor axes suggesting an intermediate ellipticity. There is minimal evidence of spiral arms or significant star formation regions. The color gradient indicates a redder central region potentially indicative of older stellar populations, while the outer regions show hints of bluer hues, possibly pointing towards pockets of younger stars. The structure displays some minor disturbances, and appears to be a relatively undisturbed system. Overall, the galaxy appears to be a fairly massive system with a relatively low star formation rate.
