The galaxy presents a primarily elliptical morphology with a high degree of central concentration. The light distribution appears smooth, with no prominent spiral arm structures visible. There is a notable color gradient, transitioning from a bright, yellowish-white core to a fainter, reddish halo. The galaxy exhibits a slight elongation, appearing nearly circular but with a discernible axis. A faint, green disturbance is observed near the center of the galaxy, indicating a possible tidal disruption or strong emission line activity. The outer regions of the galaxy gradually fade into the background sky, suggesting a smooth density profile. Overall, the galaxy appears to be a relatively massive system with an evolved stellar population.
