The galaxy presents as an elliptical morphology, appearing largely smooth and rounded. There is a concentration of light towards the center, suggesting a prominent galactic nucleus. The galaxy exhibits a subtle color gradient, transitioning from a bluish hue towards the core to a slightly redder color at the outer edges, which might indicate some ongoing, but low level, star formation. No distinct spiral arm structure is visible, though there may be some minor gravitational disturbance occurring, not suggesting a recent or ongoing major merger. The light is relatively concentrated, suggesting a moderate size. The overall appearance is consistent with a galaxy possessing a significant stellar mass, but modest star forming capacity.
