The galaxy presents an elliptical morphology with a discernible central bulge. The luminosity profile appears to be relatively smooth, showing little evidence of spiral arm structure. A distinct color gradient is observed, transitioning from a brighter, bluer core to a fainter, greener outer region. The core region is relatively compact. Faint indications of minor disturbances are possibly present in the outer regions, hinting at a past or ongoing minor merger event. The overall color indices suggest a galaxy with a mix of stellar populations. The bulk of the galaxy's light output appears to be centered around the green wavelengths, suggesting a moderate amount of star formation. However, the core also displays blue emissions, potentially indicating a population of younger, hotter stars.
