The galaxy presents as an elliptical morphology, with a smooth and featureless central bulge that appears approximately 9 kpc in diameter. The bulge exhibits a color gradient, appearing more yellow towards the center and gradually fading to a redder hue at its periphery. This color variation could indicate an aging stellar population concentrated towards the core.

The galaxy is mostly featureless, with no spiral arms or dust lanes visible within this visual range. There is little sign of active star formation within the galaxy itself. The lack of any clear distortions or tidal tails suggests that the galaxy has not undergone any recent major mergers. There is a slight but unconfirmed indication of an asymmetrical shape, deviating from a perfectly elliptical form.
