The galaxy presents as a relatively smooth, elliptical structure. Its color profile appears to transition from a yellowish-orange core to a bluer halo. The galaxy exhibits a high degree of radial symmetry, appearing mostly round. There are no obvious signs of spiral arms or a prominent disk structure. No significant tidal disturbances or signs of a major merger event are apparent. There is faint evidence of very slight disturbances to the galaxy structure. The light distribution suggests a concentrated central bulge.
