The galaxy presents a relatively smooth, elliptical morphology. The central region exhibits a concentrated, bright core, indicative of a significant stellar population density. Moving outward from the core, the light gradually diminishes, forming a diffuse halo. The overall color of the galaxy appears to be reddish-yellow, suggesting an older stellar population with a lower rate of recent star formation. There is subtle evidence of a possible minor disturbance in the outer regions, but this is fairly contained to the edges of the galaxy. The main body of the galaxy is well conserved and rounded.
