The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile with a high degree of central luminosity. The galaxy appears to have an oblate shape. The central region displays a yellow-orange hue, suggesting an older stellar population and/or dust obscuration. There is a very subtle indication of a disklike feature, but it would be difficult to classify this galaxy as a spiral. Faint hints of blue light in the disk region suggest ongoing, low-level star formation. There are no obvious signs of major disturbances or merging events in the galaxy's structure, although a minor tidal disturbance cannot be ruled out.
