The galaxy presents an overall elliptical morphology with a prominent, concentrated central bulge. The bulge exhibits a yellowish-white hue, suggesting a population of older, less active stars. Extending outwards from the central bulge, there's a fainter, more diffuse halo of bluish light, hinting at regions of ongoing star formation. The galaxy appears relatively smooth in texture with a general lack of distinct spiral arm structures. There is a slight flattening, indicating it might be an elliptical galaxy with some disc-like properties. There is evidence of an asymmetric distribution of light in the halo. It is possible that this galaxy is undergoing some sort of disturbance.