The galaxy presents as a single, relatively smooth, concentrated body with a primarily elliptical morphology. The light distribution is centrally concentrated, exhibiting a radial gradient decreasing outwards from the core. The galaxy's color profile appears to be dominated by older stellar populations, exhibiting a reddish-yellow hue. There is no obvious evidence of spiral arms or a prominent disk. There also appear to be no indications of recent major merger activity or significant tidal distortions. The lack of blue color suggests a low rate of ongoing star formation, if any.
