The galaxy presents an elliptical morphology, appearing largely smooth and featureless. The central region exhibits a concentrated, bright yellowish-orange hue, suggesting an older stellar population. Moving outwards, the galaxy displays a gradual decrease in luminosity, with a faint greenish halo extending beyond the central bulge. The overall structure suggests a lack of significant disk-like features or spiral arms. There is no apparent indication of ongoing major merger activity or significant tidal disturbances. The elongated shape indicates it is likely an elliptical galaxy with an axial ratio that departs from a perfect circle. 
