The galaxy presents as a relatively compact object with a smooth, elliptical morphology. The light distribution appears centrally concentrated, exhibiting a gradual decline in intensity from the core outwards. The galaxy appears largely featureless, lacking prominent spiral arms or distinct dust lanes. The overall color appears slightly redder in the center. This suggests an older stellar population dominates the light emission. The galaxy appears fairly isolated, showing no strong signs of tidal distortion or ongoing major merger events.
