The galaxy presents as a moderately bright, elliptical object with a smooth, featureless morphology. It exhibits a radial color gradient, transitioning from a yellow-white core to a redder outer halo. The light distribution suggests a high degree of central concentration. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or ongoing mergers. The overall color and morphology are consistent with a relatively evolved stellar population and subdued star formation activity. The observed axial ratio suggests it may be an E4-E5 type elliptical galaxy, with an apparent flattening, but further spectroscopic or photometric data are required for a more precise morphological classification.
