The galaxy presents a generally elliptical morphology, though there is evidence of a faint disk component. The central bulge is bright and appears relatively smooth, with a yellowish-white hue. The outer regions of the galaxy exhibit a bluer color, suggesting the presence of younger stellar populations, likely associated with ongoing, albeit modest, star formation. The overall structure appears relatively undisturbed, showing no prominent tidal tails or strong signs of a recent major merger event, though minor asymmetries may indicate past interactions. The galaxy appears to be relatively massive.
