The galaxy presents an elliptical morphology, with a smooth, centrally concentrated light distribution. The color gradient indicates a population of older stars, particularly in the central bulge, appearing with a yellowish hue. The isophotes are generally regular, showing a moderate ellipticity but with no prominent features indicative of spiral arms or a disk structure. There is some hint of a less concentrated, bluer halo extending beyond the central bulge. No significant signs of tidal disturbances or ongoing major merging events are apparent. 
