The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. It exhibits a high degree of roundness. There are no obvious spiral arm structures or prominent dust lanes visible. The galaxy's color profile suggests a population of older stars, with a more pronounced emission in redder wavelengths. The absence of distinct features points to a lack of recent major merger events. Faint disturbances may exist around the galaxy, although they are likely minor.
