The galaxy presents as a relatively smooth, elliptical morphology. It appears largely spheroidal in shape, with a high degree of central concentration of light. The galaxy displays a smooth light profile, indicative of an older stellar population and lacking prominent spiral arm structures or significant dust lanes. The color of the galaxy appears to be skewed toward the redder end of the spectrum. Evidence shows that there could be minor disturbances in the galaxy due to a possible merger, however, it remains largely smooth.
