The galaxy presents as a single, centrally concentrated object with a generally smooth morphology. The light distribution is relatively uniform and elliptical in shape, with a slight elongation. The color profile indicates a significant population of older stars, appearing predominantly yellow-orange. There is no obvious spiral structure or dust lane visible. The light is concentrated, suggesting that the galaxy is either viewed face on, or that it is a spheroidal galaxy. There is no evidence of any significant ongoing merger activity or tidal disturbances.
