The galaxy presents as a centrally concentrated object with a generally smooth, elliptical morphology. It appears nearly circular, exhibiting minimal deviation from a perfect sphere. While a distinct disk structure is not readily apparent, the lack of defined features suggests a relatively evolved system, potentially with a diminished rate of active star formation. There is little evidence of ongoing major mergers or significant tidal disturbances affecting the galaxy's structure. The galaxy exhibits a color gradient, appearing bluer in the central region and gradually transitioning to redder hues outwards. This color gradient is possibly indicative of radial variations in stellar populations. The galaxy appears to be a massive system.
