The galaxy presents a largely smooth, elliptical morphology. Its light distribution appears centrally concentrated with a gradual decrease in intensity outwards. The core region exhibits a bright, relatively compact luminous area, potentially indicating the presence of an active galactic nucleus or a dense concentration of stars. Color gradients are subtle, with a slight bluer hue towards the central region, which could indicate the presence of younger stellar populations or ongoing star formation. A faint, extended halo surrounds the galaxy, suggesting a substantial stellar component beyond the main body. There's a hint of minor asymmetry or disturbance in the outer regions, possibly indicating a past merger or interaction event, though it largely appears as a relaxed system. Overall, the galaxy presents characteristics of a mature, massive system with a moderate level of star formation.
