The galaxy appears to be a relatively smooth, elliptical-like object. Its color profile suggests a dominance of older stellar populations, with a pronounced yellow-orange hue. There is little evidence of prominent spiral arms or significant dust lanes. The galaxy is well-defined but appears somewhat small. The galaxy exhibits a high degree of central concentration, with the light intensity decreasing smoothly from the core outwards. There is no immediately apparent evidence of any tidal disturbances or ongoing mergers. It presents as a fairly isolated system.
