The galaxy presents a smooth, elliptical morphology. It exhibits a centrally concentrated light profile, with the highest intensity luminosity found at the core and gradually decreasing outward. The light distribution is generally smooth, with no obvious signs of spiral arm structures. The galaxy appears nearly circular in shape, with a slight deviation from perfect roundness. There is little evidence of significant ongoing star formation. The galaxy’s color appears to be trending towards redder hues. There are no obvious signs of tidal disturbances or major merger events. The galaxy's diameter is roughly 6 kpc.
