The galaxy presents a largely smooth morphology, exhibiting a dominant spheroidal structure. It appears approximately round in shape, lacking a distinct disk or spiral arm features. There is a gradual change in luminosity from the center outwards indicating a somewhat uniform distribution of stars. The galaxy's color is generally indicative of an older stellar population, with a subtle shift towards redder wavelengths in the core, potentially suggesting a concentration of older, cooler stars. The overall structure suggests minimal signs of recent mergers or significant tidal disturbances. The galaxy displays a relatively low rate of star formation.
