The galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a concentrated luminosity, appearing yellowish-white, suggesting an older stellar population dominating the central region. Moving outward from the core, there is a noticeable color gradient toward a teal hue, with fainter extended regions. This color shift indicates a potential presence of younger, hotter stars in the outer regions, though the overall star formation activity appears quite low. No distinct spiral arms or bar structures are discernible. There is a slight asymmetry, though no prominent merging signatures are evident in this image. Overall, the galaxy appears to be an evolved system with a largely quiescent star formation history, though perhaps with slightly more star formation at larger radii.
