The galaxy appears to be a relatively smooth, elliptical galaxy. Its morphology suggests an older stellar population, as evidenced by its lack of prominent spiral arms or distinct dust lanes. It exhibits a concentrated central bulge and a gradually fading, diffuse halo. The galaxy is somewhat flattened, with a slight deviation from a perfectly circular shape. The color profile indicates a redder overall hue, which aligns with the presence of older, cooler stars. There is no sign of recent or ongoing major merger activity, although a minor disturbance cannot be ruled out. The galaxy appears to be relatively isolated in its environment.
