The galaxy appears as a centrally concentrated object with a generally smooth morphology. Its overall shape approximates a rounded form, lacking a prominent disk structure. There is a slight elongation, but the galaxy does not resemble a cigar shape. The color profile suggests a relatively high emission in the green wavelengths compared to the red. There are no obvious signs of recent major merger activity or significant tidal disturbances. Faint wisps of light may be present close to the core.
