The galaxy presents as a disk-shaped structure, exhibiting a relatively smooth overall appearance. It appears to be an elliptical galaxy with a subtle disk. The light distribution suggests a high concentration of stars toward the center, with a prominent bulge region displaying a yellowish hue. The outer regions of the galaxy are less defined, with a gradual decrease in luminosity. The galaxy shows a slight deviation from perfect circularity, appearing somewhat elongated along its major axis, but is generally rounded. There are no obvious signs of a major ongoing merger, though some minor asymmetries or tidal features cannot be entirely ruled out. Based on its color, it is likely that star formation activity is relatively low.
