The galaxy appears as a single, concentrated, luminous structure. It exhibits a largely smooth, elliptical morphology, with a high degree of central concentration. The light is generally uniform, lacking strong or well-defined spiral arms or distinct features. The galaxy appears almost perfectly circular in shape. There is an apparent lack of ongoing major merging activity or significant tidal disturbances, with only a small degree of disturbance from the surrounding environment. The color profile is relatively red, suggesting an older stellar population and reduced active star formation. Based on these characteristics, the object is likely an elliptical galaxy with a red shift corresponding to approximately 17% the speed of light.
