The galaxy presents a largely smooth and concentrated morphology, suggesting an elliptical classification. The primary color is a yellowish-gold, possibly indicative of an older stellar population with fewer young, blue stars. There is a slight deviation from perfect circularity, indicating a minor degree of ellipticity. No distinct spiral arm structures or significant dust lanes are discernible within the resolution of the image. There is no apparent signs of recent or ongoing major merging activity, and the overall appearance is relatively undisturbed.
