The galaxy presents as a luminous, centrally concentrated object. Its morphology appears largely smooth and elliptical, exhibiting a high degree of circularity. There is no obvious evidence of a disk structure or spiral arms. The color profile is dominated by warmer tones, suggesting a population of older stars and a relatively low rate of current star formation. Minimal dust extinction is implied by the lack of significant color gradients across the galaxy's body. No signs of tidal disturbances or ongoing mergers are immediately apparent. It seems to be a relatively isolated system.
