The galaxy presents as a largely featureless, elliptical structure with a smooth light distribution. Its overall morphology suggests a spheroidal shape, appearing nearly circular in projection. The central region is characterized by a bright, concentrated core that gradually decreases in intensity toward the outer edges. A subtle color gradient is observed, transitioning from a yellowish-white core to a slightly redder halo. There is no apparent spiral arm structure, bar, or prominent dust lane visible. The galaxy appears to be relatively isolated, showing no signs of significant tidal interactions or major mergers. The overall structure indicates a relatively evolved system, with a high degree of symmetry and uniformity in its light profile. The overall mass is relatively large, while the rate of star formation is rather slow.
