This galaxy appears to be an elliptical galaxy, with a Sersic index indicating a high concentration of light toward the center. The galaxy exhibits a smooth, featureless morphology, lacking prominent spiral arms or a well-defined disk structure. There is some indication that there may be a secondary nucleus indicating the possibility of a recent, or ongoing, merger. Overall, this galaxy's light profile suggests an evolved system dominated by older stellar populations. The color indices suggest a redder color, consistent with a relatively passive galaxy with minimal ongoing star formation.
