The galaxy presents as a somewhat elliptical, face-on object with a smooth, centrally concentrated light profile. The central region exhibits a bright, slightly bluish-white core, suggestive of a population of young, hot stars and potential ongoing star formation, albeit at a moderate rate. The galaxy appears relatively isolated, with subtle hints of possible minor disturbances or faint tidal features. This galaxy possesses an estimated stellar mass within the range expected for intermediate-mass galaxies. The overall color suggests a mix of stellar populations, with the central region trending towards bluer colors and the outer regions appearing somewhat redder. The lack of significant spiral arm structure suggests that this is an early-type galaxy.
