The galaxy presents as a relatively smooth, rounded structure with a concentrated central bulge. The color gradient suggests a yellow-white core fading to blue-white in the outer regions, indicating a stellar population that is older in the center and younger towards the periphery. The overall form lacks well-defined spiral arms or a prominent disk, suggesting characteristics of an elliptical galaxy or a lenticular galaxy with a weak disk component. There is no evident signs of ongoing major merging events or significant tidal distortions. The galaxy appears to be relatively undisturbed and isolated.
