The galaxy appears to be a relatively compact elliptical or lenticular galaxy, exhibiting a largely smooth and featureless morphology. There is a central concentration of light suggesting the possible presence of a galactic nucleus. The overall color appears to be redder, implying a population of older stars, although some bluer light is observable. The galaxy appears isolated, with no obvious signs of tidal disturbances or major ongoing mergers. The overall shape of the galaxy appears to be mostly round, with a slight ellipticity. The galaxy shows no apparent signs of strong spiral arm structure or active star formation regions.