This galaxy presents as an elliptical morphology, exhibiting a smooth, relatively featureless light distribution. There is a concentrated central bulge, which gradually fades into a diffuse halo. The galaxy appears generally round, with a slight deviation suggesting a possible intermediate ellipticity. Color gradients are subtle, with a slightly yellower hue towards the core transitioning to a bluer tinge in the outer regions. This suggests a stellar population gradient, possibly indicating older, redder stars concentrated in the center and younger, bluer stars distributed further out. There are no obvious signs of tidal disturbances or ongoing mergers. Overall, the galaxy appears to be a mature system with a relatively quiescent star formation rate.
