The galaxy presents as a fairly compact, elliptical morphology. It exhibits a smooth, centrally concentrated light distribution with a high degree of radial symmetry. The color gradient suggests a relatively older stellar population, with a yellow/orange hue dominating the central region, indicative of evolved stars. There is a faint blueish halo surrounding the center. No prominent spiral arms or significant dust lanes are discernible. There is no indication of a major ongoing merger event, though minor tidal features or disturbances cannot be ruled out at this resolution. The galaxy appears to be generally quiescent in terms of star formation activity, consistent with its smooth morphology and redder colors.
