The galaxy presents a largely smooth, elliptical morphology. It exhibits a bright, concentrated central bulge, appearing approximately round in shape. The overall color profile suggests a relatively old stellar population, with a dominant yellowish-orange hue in the core region. There may be a faint hint of bluer light in the outer regions, potentially indicative of some ongoing, albeit low-level, star formation. No distinct spiral arms or prominent features are discernible. There is no visually obvious tidal disruption or signs of recent merger activity in the immediate vicinity of the galaxy. 
