The galaxy presents a generally smooth, elliptical morphology. The light distribution indicates a significant central bulge component, exhibiting a yellowish-orange hue, suggesting a population of older, evolved stars. Fainter, bluish regions extend outwards from the central bulge, possibly indicating regions of ongoing, albeit limited, star formation. There is no clear evidence of spiral arms or a well-defined disk structure. The overall shape is moderately round, with no apparent tidal features or major disturbances suggesting recent merger activity. There might be slight asymmetry to the galactic halo surrounding the central bulge.
