The galaxy appears as a relatively smooth and centrally concentrated object. It exhibits a primarily elliptical morphology, with a moderate degree of ellipticity that leans toward round. The central region shows a high surface brightness, suggesting a significant concentration of stars. The galaxy's color profile shifts subtly from a yellowish-white core to slightly bluer outer regions, hinting at potential variations in stellar populations or ongoing star formation. There is no strong indication of spiral arm structure or a prominent disk component. Faint distortions are present in the galaxy's outer envelope, which might imply minor gravitational interactions, although these do not represent a major disturbance.
