The galaxy appears to be a relatively smooth, elliptical system. Its overall color profile indicates an older stellar population, with a yellowish-orange hue dominant throughout the galaxy's body. There's a slight concentration of light towards the center, indicating a possible galactic nucleus, but no distinct features such as spiral arms or a bar structure are discernible. The lack of prominent blue regions suggests limited ongoing star formation within the visible portion of the galaxy. The morphology leans towards a near-spherical shape, with only a subtle deviation towards a more elongated form. There is no evidence of major disturbances.