The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a high degree of luminosity, suggesting a dense concentration of stars and potentially an active galactic nucleus, though further spectroscopic analysis would be needed to confirm this. The color profile shows a subtle gradient from a bluer hue in the outer regions towards a redder core, which may indicate a younger stellar population in the galactic outskirts and an older, more evolved population towards the center. There may be minor disturbances or interactions that can be observed with slight asymmetries in the galaxy's outer halo.
