The galaxy presents as a concentrated spheroid, exhibiting a smooth, featureless morphology, likely an elliptical galaxy. The core displays a bright, golden hue, suggestive of an older stellar population. The light distribution appears concentrated towards the center, indicating a high degree of central mass concentration. There is a slight ellipticity to the galaxy's overall shape, appearing somewhat rounded and only slightly cigar-shaped. There is no discernible dust lane, spiral arm structure, or ongoing major merger activity visible in the image. Faint color variations are present in the outer regions, possibly indicating subtle changes in stellar population or metallicity, but there is no strong evidence of active star formation. The galaxy appears undisturbed, not showing signs of recent interaction with other galaxies.
