The galaxy presents as a relatively smooth, elliptical object with a somewhat elongated shape. The color profile suggests a dominant older stellar population, displaying a central yellowish hue, indicative of evolved stars. There is a subtle hint of bluer color in the outer regions, possibly indicating some degree of ongoing, though relatively subdued, star formation. No strong spiral arm structures or significant dust lanes are apparent. There is also no visible evidence of a major ongoing merger. There appears to be a slight disturbance in the morphology suggesting a possible minor disturbance.
