The galaxy appears to be elliptical in morphology, with a smooth, centrally concentrated luminosity profile. It exhibits a yellowish-orange hue, suggesting an older stellar population with relatively little ongoing star formation. The galaxy appears relatively undisturbed, without prominent tidal features or signs of a recent major merger. There is a hint of a slight elongation or deviation from perfect circularity in its shape, potentially indicating a minor interaction or internal dynamics. The color suggests a high mass galaxy.
