The galaxy presents a largely smooth and rounded morphology, suggesting a classification as an elliptical galaxy or possibly a lenticular galaxy seen face-on. There is very little evidence of spiral arms or prominent disk-like structure within the observable wavelengths. The light distribution is centrally concentrated. The galaxy's color is generally redder, indicative of an older stellar population and lower levels of ongoing star formation. There is a subtle bluer gradient that may suggest some young population of stars or some small amount of star formation taking place. There is no apparent evidence of major tidal disturbances or strong interactions with neighboring galaxies. The overall impression is one of relative quiescence and morphological stability.
