The galaxy presents as a large, centrally concentrated object with a smooth, relatively featureless morphology. It appears to be elliptical in shape, exhibiting a high degree of sphericity with only a slight deviation from a perfectly circular form. A bright, compact core is visible, suggesting a concentration of stars toward the center of the galaxy. The light profile gradually fades from the center outwards, indicating a decrease in stellar density with increasing distance from the nucleus. The galaxy shows a subtle color gradient, appearing slightly bluer in the outer regions than in the core, which could be indicative of younger stellar populations or ongoing star formation in the outer parts, however, star formation is expected to be low. There is no apparent spiral arm structure, bars, or dust lanes visible in this image. Overall, the galaxy appears to be an evolved system, likely dominated by older stellar populations.
