The galaxy presents as a relatively well-defined, though somewhat diffuse, structure with an apparent edge-on disk morphology. The central bulge exhibits a distinctly rounded profile. There is a slight hint of boxiness to it, but the rounded appearance is dominant. Dust lane obscuration appears minimal, based on what looks like the absence of an apparent dark band bisecting the galaxy. Overall, the galaxy appears relatively undisturbed, with no readily apparent signs of major merging activity or significant tidal distortions. The lack of prominent blue regions suggests low ongoing star formation and redder colors for older stellar populations. The galaxy appears to be relatively massive.
