The galaxy presents as an elliptical morphology, appearing largely smooth and well-rounded with no readily discernible spiral arms or distinct features. Its light profile exhibits a concentrated central region which gradually diffuses outwards. The dominant color is a broad spectral type with an approximate blueish-white hue to it. The observed color and smooth morphology may indicate an older stellar population with ongoing star formation. There is no evidence of significant tidal disturbances or active galactic nuclei based on this image alone.
