The object presents as a galaxy with a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that appears bright and slightly blue-white in color, suggestive of an older stellar population with ongoing star formation. The surrounding halo is more diffuse and less luminous, exhibiting a bluer hue. The galaxy appears to be fairly isolated, without obvious signs of tidal interactions or major disturbances indicating a recent merger, though a hint of asymmetry in the outer regions might suggest minor gravitational interactions in the past. Overall, the galaxy seems to be relatively evolved. 
