The galaxy presents as a centrally concentrated, smooth structure. It appears elliptical in shape, exhibiting a gradual decline in luminosity from a bright, yellowish core outwards to a more diffuse, fainter halo. No distinct spiral arm structures are discernible. There may be some slight asymmetry, but no significant tidal features or signs of ongoing mergers are evident. Color gradients suggest the core may be populated with older stellar populations. There is a hint of bluer stars located on the outskirts of the main elliptical body, indicating ongoing or recent star formation.
