The galaxy presents as a roughly elliptical structure with a fairly smooth overall appearance. The central region exhibits a higher surface brightness, suggesting a concentration of stars toward the core. The light profile appears relatively even, transitioning gradually from the bright core to the fainter outer regions. There is some evidence of blue tinges throughout the galaxy. The galaxy appears relatively isolated, exhibiting no obvious signs of strong tidal interactions or major mergers, though there is some suggestion of minor disturbance in its shape.
