The galaxy presents as a centrally concentrated system, exhibiting a dominant bulge component. Its morphology appears to be largely smooth, with a high degree of central symmetry. The light profile suggests a relatively uniform distribution throughout the main body of the galaxy. Some slight asymmetry is present, but it is minimal. Color gradients are apparent, showing a yellowish-white core, possibly indicating an older stellar population and lower star formation rates. The outer regions of the galaxy exhibit fainter, bluer hues, which might indicate the presence of younger stars. There is no clear evidence of spiral arms or a prominent disk. The galaxy appears relatively undisturbed, with no signs of significant tidal interactions or ongoing mergers, though subtle minor disturbances might be present.
