The galaxy presents an elliptical morphology, appearing relatively smooth with a high degree of central concentration. The light distribution suggests a dominant spheroidal component. The axial ratio indicates a moderate degree of ellipticity, tending towards an elongated shape rather than a perfect sphere. There may be some faint hints of a disk component, although this is not well-defined. There is no obvious evidence of spiral arms or a bar. Color gradients suggest a redder core, indicative of an older stellar population and possibly dust attenuation. No major signs of ongoing mergers are visible, but minor disturbances or tidal features cannot be completely ruled out. The overall appearance is consistent with a mature galaxy with a suppressed star formation rate.
