The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology suggests a spheroid-dominated system, possibly an elliptical galaxy or a lenticular galaxy viewed close to face-on. There is a distinct color gradient, with the central region appearing more yellow, potentially indicating an older stellar population and less ongoing star formation activity. The outer regions show hints of bluer colors, possibly indicating the presence of younger, hotter stars, but overall the galaxy lacks prominent spiral arm structures or distinct features usually associated with actively star-forming disk galaxies. The roundness is moderate. There are no apparent signs of major tidal disturbances or ongoing merging activity, although subtle irregularities in the outer regions cannot be ruled out at this resolution. 
