The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, appearing mostly round. There is a noticeable color gradient, with the central region displaying a yellowish-white hue, transitioning to a bluer tint in the outer regions. No distinct spiral arms or other prominent features are discernible. The overall appearance suggests a system dominated by an older stellar population, though some ongoing star formation is evident. There are no signs of major disturbances or interactions with other galaxies in the immediate vicinity. Faint hints of a disk-like structure may be present, but the spheroid component dominates the observed morphology.
