The galaxy appears to be a relatively smooth, elliptical system. Its light is centrally concentrated, exhibiting a radial gradient decreasing in intensity from the core outwards. The galaxy presents a generally round morphology, lacking any prominent features such as spiral arms or a distinct disk. There's no evidence of ongoing major merging activity or significant tidal disturbances in the immediate vicinity. The galaxy exhibits a color profile indicative of an older stellar population. It appears as a relatively quiescent system with limited star formation.
