The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile with a gradual decrease in brightness towards the outer regions. The core is bright and has a yellow hue, suggesting an older stellar population. There is a faint bluish halo around the bright yellow center. The overall shape is close to round, with no obvious signs of strong tidal disturbances or ongoing major mergers. Faint, subtle irregularities in the outer regions may indicate past minor interactions, but the galaxy is largely undisturbed. 
