The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal in shape with a concentrated central bulge. It displays a gradual radial decrease in luminosity. There's a slight color gradient, with the core exhibiting a yellower hue, suggesting an older stellar population, transitioning to a slightly bluer periphery which could indicate some younger stars present, though subdued. There is no apparent spiral arm structure or significant dust lane visible, however, it is relatively compact, showing no indication of major ongoing mergers or significant tidal disturbances.
