The galaxy presents as a largely smooth, elliptical-like structure. Its core exhibits a concentrated luminosity, gradually diminishing towards the outer regions. The color profile suggests a relatively evolved stellar population, with a dominant yellowish-white hue, indicative of older stars. There is a slight asymmetry visible in the outer regions. There's a hint of a faint, extended halo surrounding the main body of the galaxy. There does not appear to be a significant presence of dust lanes or prominent star-forming regions within this galaxy. The overall morphology implies it is likely a galaxy that has undergone significant evolution, possibly through mergers or secular processes.
