The galaxy appears as a centrally concentrated, relatively smooth object. It exhibits a generally elliptical morphology, appearing quite rounded in its overall shape. There is little evidence of spiral arm structures or distinct features, the light appears to be diffuse and consistent across the galaxy. The color gradient suggests a redder core transitioning to slightly bluer hues in the outer regions, although the bluer regions are not strongly defined. The smoothness and color profile suggest a galaxy dominated by an older stellar population, with ongoing, but possibly reduced, star formation activity. There does not appear to be evidence of any recent major merger events or significant tidal disturbances. Overall, the galaxy is consistent with a relatively evolved system, likely an elliptical or S0 galaxy.
