The galaxy presents as a primarily smooth, elliptical morphology. There is a centrally concentrated bulge with a yellowish hue, suggesting an older stellar population. The outer regions exhibit a slightly more diffuse greenish coloration, potentially indicating the presence of some younger stars or ongoing, albeit low, levels of star formation, particularly in the central region. The galaxy appears to be relatively undisturbed, showing no obvious signs of recent merger activity. The round appearance could indicate the galaxy is more face-on, but could also point to a spherical shape typical of elliptical galaxies. Overall, the galaxy seems to be a relatively massive, quiescent system.
