The galaxy presents as an elliptical system with a moderately smooth, diffused morphology. Its color gradients suggest an older stellar population, evidenced by the central concentration of redder hues, likely indicative of evolved stars. Fainter greenish hues are observed in the outer regions of the galaxy, which may point to the presence of ongoing, low-level star formation activity. A hint of spiral structure or a disk is not clearly discernible from the image but some minor features may indicate this. There is a strong possibility of a recent interaction or merger as the morphology does not appear completely relaxed and undisturbed. Overall, the galaxy appears to be a relatively massive system with a moderate degree of central condensation.
