The galaxy presents an elliptical morphology, appearing as a somewhat flattened spheroid. The central region exhibits a high concentration of light, suggesting a prominent bulge component. A fainter, bluer structure is visible near the galaxy, indicating possible tidal interaction or a merging event with a smaller companion galaxy. This blue region implies ongoing star formation. The overall color gradient from the core outwards suggests an aging stellar population in the central regions and relatively younger stars in the outer regions. A faint stellar halo extends outwards from the main body. The galaxy displays signs of morphological disturbance, potentially caused by past or ongoing interactions.
