The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. The central bulge exhibits a yellowish hue, suggestive of an older stellar population. A fainter, bluer halo surrounds the core, potentially indicating some degree of recent star formation in the outer regions, although it could also be attributed to scattering. The galaxy presents with an elongated shape, likely an elliptical shape that is oriented at an angle relative to the viewer, and appears to exhibit no major distortions or signs of ongoing mergers, although faint disturbances cannot be ruled out at this resolution. The galaxy seems to be relatively isolated in its environment.
