The galaxy appears as a relatively smooth, elliptical form, with a high degree of central concentration. The light profile suggests a gradual decline in surface brightness moving outwards from the core. There is a slight elongation, possibly indicating it's an elliptical galaxy of type E4-E5. The overall color is yellowish-orange. This color suggests an older stellar population with lower ongoing star formation. There is no evidence of spiral arms or significant dust lanes and the overall morphology suggests a lack of major recent mergers or tidal disturbances. Some low-level blue light is visible in the outskirts, potentially indicative of some recent, albeit minimal, star formation activity. 
