The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness towards its outer regions. The galaxy's overall shape is largely circular, showing only a slight deviation from perfect sphericity. There is no indication of a distinct disk or spiral arms. 

The galaxy exhibits a subtle color gradient, appearing slightly bluer in the central region, suggesting the presence of a younger stellar population within the core, but it is mostly dominated by redder colors. No signs of active galactic nuclei, such as jets or strong emission lines, are readily apparent. The galaxy does not appear to be undergoing a major merger or tidal interaction with another galaxy, and shows no clear evidence of significant morphological disturbance. Based on the color and smooth morphology, the galaxy is likely a relatively massive and evolved system with moderate star formation.
