The galaxy appears as a centrally concentrated, elliptical-like structure. Its color profile suggests a dominant population of older stars, giving it a yellowish-orange hue. The galaxy exhibits a high degree of smoothness, with no apparent spiral arms or distinct features such as dust lanes or star-forming regions. It has a generally rounded morphology, showing no significant elongation or distortion. There is no visual evidence of ongoing or recent merger activity; the galaxy seems relatively undisturbed. The galaxy has moderate luminosity.
