The galaxy appears to be a relatively smooth, elliptical structure with a distinct central bulge. The light is concentrated towards the center, indicating a higher density of stars in that region. The galaxy exhibits a moderate ellipticity, appearing somewhat elongated. Color gradients are subtle, with the central region appearing slightly more yellow/orange than the outer regions, suggesting an older stellar population centrally concentrated. There is no visible evidence of spiral arms or significant dust lanes. No signs of any major ongoing merger activity are present.
