The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, relatively featureless morphology. The central bulge is prominent and displays a yellowish hue, indicative of an older stellar population. Moving outwards from the core, the luminosity gradually decreases. There's no readily apparent spiral arm structure or significant dust lane obscuration. The galaxy appears somewhat elongated, but generally rounded in shape. Faint extensions or tidal features cannot be decisively ruled out, though no major distortions are observed. The overall color profile suggests ongoing, but relatively low, levels of star formation activity.
