The galaxy presents as a central, concentrated luminosity, with a predominantly smooth morphology. The galaxy's shape appears elliptical, with its light gradually diminishing from the core outwards, suggesting an older stellar population. There is no evident spiral arm structure. The galaxy exhibits a yellowish-red hue, indicative of a population of older, cooler stars. There is no distinctive color gradient or patchiness within the galaxy's halo. The light distribution appears relatively uniform, with no indications of any recent major mergers or significant tidal disturbances. There might be a slight elongation observable along one axis, making it "in between" round. There is a low presence of any active star formation.
