The galaxy presents as a single, dominant, spheroidal structure. It exhibits a smooth, relatively featureless morphology, lacking prominent spiral arms or a well-defined disk. The light distribution appears concentrated towards the center, suggesting a prominent bulge. The galaxy displays a yellowish-orange hue, possibly indicating an older stellar population with lower levels of recent star formation. The overall shape approximates a circular form, with a slight suggestion of ellipticity. There is no apparent sign of ongoing major merger activity or significant tidal disturbances.
