The galaxy appears as a centrally concentrated, elliptical-like structure. It presents a smooth, largely featureless morphology. The light distribution suggests a relatively high degree of symmetry, though there is a slight elongation. The galaxy exhibits a color gradient, with a brighter, yellower core, transitioning to a slightly fainter, more reddish halo. There is no apparent spiral arm structure or dust lanes. The overall color indicates an older stellar population. There is no strong evidence of ongoing major merger activity. Small disturbances cannot be ruled out.
