The galaxy presents as a roughly elliptical, unresolved central bulge with a relatively smooth texture. A faint, extended halo surrounds the central region with a subtle greenish tint, suggesting possible ongoing, low-level star formation. There is minor evidence of faint, blue structures emanating from the core, potentially indicative of faint spiral arms or tidal disturbances. Overall, the galaxy appears fairly isolated and lacks significant signs of interaction, although minor asymmetry indicates a very slight disturbance. The concentration of light is strongest in the center and gradually decreases with radial distance.
