The galaxy appears to be a relatively smooth, elliptical galaxy, with a concentrated central bulge and a diffuse halo. The light profile suggests a higher concentration of stars towards the center, fading gradually outwards. The galaxy exhibits a slight ellipticity, appearing somewhat rounded but not perfectly spherical. There's no clear indication of spiral arm structure or significant dust lanes, suggesting an older stellar population. Overall, the galaxy's morphology points towards a more evolved system, possibly experiencing a low star formation rate.
