The galaxy presents as a centrally concentrated, yellowish-white elliptical. It exhibits a smooth, featureless morphology, lacking prominent spiral arms or a distinct disk. The radial light profile suggests a high degree of central concentration, transitioning to a more diffuse outer halo. The galaxy appears generally rounded with a slight elliptical elongation. There is no visually apparent evidence of ongoing major mergers or significant tidal disturbances. Based on the galaxy's color, it likely consists predominantly of an older stellar population. Star formation activity appears to be minimal.
