The galaxy appears as a single, relatively smooth object with a concentrated central bulge. The light profile suggests a centrally dominant, spheroidal morphology with a diffuse, extended halo. The color gradient shows a shift from bluer hues in the outer regions to a redder core. There is no prominent spiral arm structure or significant dust lane obscuration visible. The galaxy is fairly isolated, showing no obvious signs of interaction or disturbance. The lack of distinct morphological features suggests it is an evolved galaxy, possibly an elliptical or lenticular type. There is very little evidence of ongoing star formation.
