The galaxy presents an overall elliptical morphology, appearing largely smooth in texture with a high degree of central concentration. The primary body of the galaxy exhibits a bright, yellowish-white core, suggesting a significant population of older stars. There appears to be a slight elongation, exhibiting a cigar shape, rather than being perfectly spherical. The outer regions of the galaxy fade into a faint blueish halo. No distinct spiral arm structures are observed. The galaxy appears isolated, with no clear indications of a major ongoing merger, though a minor disturbance may be present. Overall, the galaxy appears as a relatively evolved system.
