The galaxy presents as a smooth, centrally concentrated object with an elliptical morphology. It exhibits a high degree of symmetry, with a relatively gradual decline in surface brightness from the core outwards. The light profile appears flattened but elongated, deviating moderately from a perfect circular shape. The central region is considerably brighter and displays a bluish hue, suggestive of a population of young, hot stars and ongoing star formation, especially in the central regions. The outer regions appear redder, indicating an older stellar population. No distinct spiral arms or prominent dust lanes are visible. There is a subtle hint of asymmetry and potentially a minor disturbance in the structure.
