The galaxy presents as a generally smooth, elliptical-like structure. The central region exhibits a concentrated luminosity, appearing nearly spheroidal. The light distribution fades gradually outwards from this central region, without any distinct spiral arm features or prominent dust lanes visible. The overall color profile suggests a significant population of older stars, given the dominant yellowish-red hue in the core, and the presence of a lower level of star formation activity is suggested by the somewhat bluer outer regions of the galaxy. There is no apparent evidence of recent major merger activity or significant tidal disturbances, though some minor asymmetry in the outer halo cannot be ruled out. The galaxy exhibits moderate roundness, appearing neither perfectly spherical nor highly elongated.
