The galaxy presents as a concentrated spheroid of light, exhibiting a smooth and relatively featureless appearance. The color profile suggests a higher concentration of older stellar populations, most notably in the central bulge, indicated by the yellowish hue. There is a marginal suggestion of a surrounding disk, but this structure contributes negligibly to the overall morphology. The overall roundness is somewhat ambiguous, appearing somewhere between being fully circular and ellipsoidal. There is no apparent evidence of ongoing mergers or significant tidal disturbances, though the faintness of outer regions makes subtle disturbances hard to detect. Given the color profile and lack of prominent spiral structure, the galaxy most likely exhibits a low star formation rate. 
