The galaxy appears as a centrally concentrated, elliptical system, with a smooth light profile indicative of an older stellar population. The core exhibits a bright, yellowish hue, possibly indicating the presence of a population of evolved stars, or dust obscuration in the central region. Moving outward from the center, the light becomes more diffuse, with a slight color gradient trending towards redder hues in the outer regions. There's little evidence of spiral arms or distinct features like star clusters. Overall, the galaxy's morphology is consistent with an early-type galaxy in a relatively quiescent state, showing minimal signs of recent star formation or merger activity. A slight elongation is visible.
