The galaxy presents an elliptical morphology, though with some visible disturbance. The central region displays a yellow hue, likely indicating an older stellar population. A distinct redder, compact region is observed offset from the center, suggesting possible active star formation or a heavily obscured nucleus. There is a faint bluish halo, possibly indicative of younger stars or tidal debris. Given the asymmetry and the potential presence of disturbed features, further investigation into its interaction history or internal dynamics is warranted.
