The galaxy presents a primarily smooth, elliptical morphology with a high degree of central concentration. It exhibits a roughly spherical profile with a minor asymmetry. The color profile suggests a relatively old stellar population. The central region displays a slightly redder hue, potentially indicative of a higher density of older, cooler stars, or dust obscuration. The outer regions appear bluer, possibly indicating ongoing, albeit weak, star formation. No prominent spiral arms or bar structures are discernible. There is a subtle indication of minor disturbance or tidal features in the immediate vicinity, but these are not conclusive signs of a recent major merger event. Overall, the galaxy appears to be a relatively isolated, evolved system transitioning toward a more quiescent state.
