The galaxy presents as a generally smooth, elliptical structure. It exhibits a bright, concentrated central bulge that transitions into a less defined, extended halo. The light profile suggests a relatively even distribution of stellar populations throughout the galaxy, with a slight concentration of older, redder stars towards the center, giving the core a yellowish hue. The outer regions appear somewhat bluer, hinting at the presence of younger stellar populations or ongoing, but low levels of star formation. There's a subtle asymmetry in the outer regions, possibly indicating a past minor interaction or disturbance. No prominent spiral arms or distinct dust lanes are observed. The overall appearance is consistent with an evolved galaxy, potentially in the process of quenching star formation.
