The galaxy appears to be a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that gradually fades into a diffuse halo. The core region displays a yellowish hue, possibly indicating an older stellar population. The outer regions of the galaxy seem slightly bluer, potentially signifying the presence of younger stars or ongoing, albeit low-level, star formation. No prominent spiral arms or dust lanes are discernible in this image. There is no evidence of major tidal disturbances or ongoing mergers; however, a slight asymmetry may be observed. Overall, the galaxy presents a well-defined, spheroidal morphology with a smooth light distribution.
